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© Scott A. Southern, Ottawa, Canada, 2016
Investigations of Non-Covalent Carbon Tetrel Bonds by
Computational Chemistry and Solid-State NMR Spectroscopy
Scott Alexander Southern
A thesis submitted to the Faculty of Graduate and Postdoctoral Studies in
partial fulfillment of the requirements for the degree of
Master of Science
Ottawa-Carleton Chemistry Institute
Department of Chemistry and Biomolecular Sciences
Faculty of Science
University of Ottawa
II
Table of Contents
List of Figures ............................................................................................... IV
List of Tables .................................................................................................. X
Abstract ...................................................................................................... XIII
Acknowledgements ..................................................................................... XV
Statement of Originality ............................................................................. XIX
Chapter 1 - Introduction .................................................................................. 1
1.1 The Basic Properties of Matter ................................................................. 1
1.2 Noncovalent interactions ........................................................................... 5
1.2.1 Sigma-Holes .................................................................................................... 8
1.2.2 Sigma Hole Bonding ..................................................................................... 11
1.3 Group IV “Tetrel” Bonding .................................................................... 13
1.4 Nuclear Magnetic Resonance Spectroscopy ........................................... 17
1.4.1 The Zeeman Interaction ................................................................................ 17
1.4.2 Magnetic Shielding ....................................................................................... 22
1.4.3 Spin-spin coupling ........................................................................................ 24
1.4.4 Other NMR interactions ................................................................................ 25
1.5 Objectives ................................................................................................ 26
Chapter 2 - Instrumentation and Methodology ............................................. 28
2.1 Sample Preparation ................................................................................. 28
2.1.1 Introduction to Theoretical Aspects of Powder X-Ray Diffraction .............. 28
2.2 Quantum Computational Chemistry ....................................................... 29
2.2.1 The Hartree-Fock Method and the Self Consistent Field .............................. 29
2.2.2 Møller-Plesset Perturbation Theory .............................................................. 35
2.2.3 Density Functional Theory ............................................................................ 36
2.2.4 Computation of NMR Parameters using DFT............................................... 40
2.2.5 Gauge Including Projector Augmented Wave DFT Calculations ................. 41
2.2.6 Counterpoise Correction ............................................................................... 42
2.3 Experimental Methodology of SSNMR .................................................. 43
2.3.1 Experimental Setup ....................................................................................... 43
2.3.2 Magic Angle Spinning .................................................................................. 45
III
2.3.3 Sensitivity Enhancement ............................................................................... 46
2.3.3.1 Cross-Polarization ............................................................................................. 46
2.3.3.2 Data Acquisition Periods .................................................................................. 48
2.4 Experimental Methods ............................................................................ 49
2.4.1 Sample Preparation ....................................................................................... 49
2.4.2 Powder X-ray Diffraction – Experimental Methods ..................................... 50
2.4.3 Cluster Model Analysis ................................................................................. 50
2.4.4 Solid-State NMR ........................................................................................... 52
2.4.5 GIPAW DFT ................................................................................................. 52
Chapter 3 - Results and Discussion ............................................................... 54
3.1 Computational Investigations of NMR Trends in Tetrel Bonds ............. 54
3.2 Experimental NMR Investigations of Noncovalent Tetrel Bonds .......... 70
Chapter 4 - Conclusions ................................................................................ 83
References ..................................................................................................... 85
Appendix I – Supplementary Data .............................................................. 103
Appendix II – Sample of Computation Input Files ..................................... 121
Gaussian Input for the Geometry Optimization of Acetylene ........................ 121
Gaussian Input for NMR calculation of Magnetic Shielding Contributions .. 122
Gaussian Input for NMR calculation of J-coupling ........................................ 123
IV
List of Figures
Figure 1. A basic representation of a 12C atom using the Rutherford-Bohr model. The nucleus
(blue) is surrounded by the orbit of electrons occupying two energy levels. Two
electrons (yellow) reside in the n=1 shell, and four in the n=2 shell. Note that
further electronic orbitals may exist beyond those that are occupied in the case of
an excited electronic state. .................................................................................... 2
Figure 2. The electronic configuration diagram for a single fluorine atom (1s22s22p5). The
filling of the molecular orbitals, with increasing energy, follows Hund’s rule. ... 4
Figure 3. The hydrogen bond. The electrostatic interactions between the partially positive
(δ+) and partially negative (δ-) charge contribute to an attractive interaction
between the oxygen and hydrogen atoms in water molecules. ............................. 6
Figure 4. The electrostatic potential at the 0.001 a.u. surface of various structures exhibiting
σ-holes. The σ-hole is present on (b) chloromethane; (c) fluoromethane; (d) a
methyl group that is covalently bonded to methylammonium. For illustration
purposes, a molecule of methane (a) is shown and does not to possess a sigma hole
on carbon. Instead, the area where the hole ought to be is more negative due to
the electronic depletion over the hydrogen atoms (each of which coincidently
possess a single hole15). The red colour corresponds to electrostatic potential
values ≤ 0.172 a.u. and the blue colour corresponds to electrostatic potential values
≥ 0.179 a.u. .......................................................................................................... 10
Figure 5. General schematic of a tetrel bond, where R is a covalently bonded atom or
functional group, X is the tetrel bond donor (X = C, Si, Ge, Sn, or Pb), and Y is
V
the tetrel bond acceptor.40 dX-Y is smaller than the sum of the van der Waals radii
of the interacting atoms. ...................................................................................... 12
Figure 6. (a) The electrostatic potential at the 0.001 au surface of positively charged
dimethylammonium (left) and formaldehyde (centre) computed by CAM-
B3LYP/6-311++G(d,p). The red colour on dimethylammonium (right)
corresponds to electrostatic potential values ≤ 0.172 au; the blue colour
corresponds to electrostatic potential values ≥ 0.179 au. The -hole is present on
the methyl carbon and is adjacent to the C-N -bond, and it has an electrostatic
potential value of 0.179 au. (b) A carbon tetrel bond involving a methyl carbon.
(c) An example of a carbon tetrel bond occurring in the crystal structure of
sarcosinium tartrate. ............................................................................................ 14
Figure 7. A schematic showing the influence of a tetrel bond on the activation of an SN2
reaction. Inspired from the work of Grabowski.56 Purple: fluorine; Grey: carbon;
White: hydrogen; and Yellow: chlorine. ............................................................. 15
Figure 8. The Zeeman Effect for a spin-½ nuclide. The splitting of the spin states is observed
as a function of the strength of the magnetic field. ............................................. 20
Figure 9. A 9.4 T NMR spectrometer magnet for the solid state. The superconducting coil is
found within the large cylindrical container, which also houses the cooling liquid.
............................................................................................................................. 44
Figure 10: Typical single pulse cross polarization pulse program. A 𝜋
2 pulse is applied to the
proton channel, followed by a 1H 13C contact time. This is followed by the
acquisition period coinciding with decoupling from the protons. ....................... 48
VI
Figure 11. The increase of the signal-to-noise ratio as a function of the number of time
dependent scans. Initially, the signal intensity grows rapidly, but as time continues
to increase, the interval at which the signal gain is achieved becomes impractically
long. ..................................................................................................................... 49
Figure 12. A 4 mm MAS rotor compared to a Canadian Penny for scale. The cap of the rotor
is winged so that it may spin using a high pressure air stream. The spinning speed
is adjusted using an MAS controller fit onto the spectrometer console. ............. 52
Figure 13. Cost analysis of the various methods used in the test study on model 6. The red
hashed line represents the energy difference cut-off for this study at 0.5 kcal/mol,
as compared to the energy obtained in the QCISD calculation. All energies are at
a tetrel bond distance of 2.825 Å. The time taken for the QCISD calculation was
5,232 s. ................................................................................................................ 56
Figure 14. Model compounds containing carbon tetrel bonds between methyl carbons and
oxygen-containing functional groups. ................................................................. 57
Figure 15. A schematic showing how the tetrel bond lengths of the model compounds are
modified for the computations. The bond lengths are changed in 0.10 Å increments
from 2.825 Å to 3.325 Å. The atomic coordinates are modified in the GaussView
software. .............................................................................................................. 58
Figure 16.. NMR computational investigations of model compounds. Calculated isotropic
chemical shifts of model compounds using (a) MP2, (b) B3LYP, (c) LC-PBE,
(d) LC-PBE-D3, (e) BHandHLYP, and (f) CAM-B3LYP are plotted against the
reduced distance parameter (rC∙∙∙Y) (top axis) and the interaction distance (d
VII
(C∙∙∙Y)) (bottom axis). Each plot is fit by a quadratic polynomial function with R2
> 0.99 for all methods except CAM-B3LYP (Table 12-Table 17). For spacing,
data values for structures 8, 9, 13 and 14 are found in Table 6 to Table 8 in
Appendix I – Supplementary Data. ..................................................................... 60
Figure 17. Computed CP corrected interaction energy values vs. interaction distance of the
model compounds. Computed interaction energies using (a) MP2, (b) B3LYP, (c)
LC-PBE, (d) LC-PBE-D3, (e) BHandHLYP, and (f) CAM-B3LYP are plotted
against the reduced distance parameter (rC∙∙∙Y) (top axis) and the interaction
distance (d(C∙∙∙Y)) (bottom axis). The calculated interaction energies of the model
compounds were obtained by 6-311G++(d,p) with each respective functional.
Each plot is fit by a quadratic polynomial function with R2 > 0.96 (Table 12 to
Table 17 in Appendix I – Supplementary Data). ................................................ 64
Figure 18. Computed J-coupling for model compounds. Graphs represent 1cJ-coupling
values between 13C and either 17O or 15N using (a) The LC-PBE-D3, (b)
BHandHLYP, and (c) CAM-B3LYP methods. In each case, the 6-311++G(d,p)
basis set is used. Each plot is fit by a quadratic polynomial function with R2 > 0.99
(Table 9 to Table 11 in Appendix I – Supplementary Data).............................. 70
Figure 19. The tetrel bond present in N,N,N’,N’-tetramethylethylenediammonium succinate
succinic acid. The interaction distance is 3.07 Å. ............................................... 71
Figure 20. Powder X-Ray diffractogram of sarcosine. The simulated diffractogram (a) was
obtained using the Mercury version 3.5.1 software provided by the CCDC. The
VIII
experimental diffractogram (b) was obtained from a powdered sample using a
Rigaku Ultima IV X-ray diffractometer. ............................................................. 73
Figure 21. Powder X-Ray diffractogram of sarcosinium tartrate. The simulated
diffractogram (a) was obtained using the Mercury version 3.5.1 software provided
by the CCDC. The experimental diffractogram (b) was obtained from a powdered
sample using a Rigaku Ultima IV X-ray diffractometer. .................................... 74
Figure 22. Powder X-Ray diffractogram of N,N,N’,N’-tetramethylethylenediammonium
dichloride. The simulated diffractogram (a) was obtained using the Mercury
version 3.5.1 software provided by the CCDC. The experimental diffractogram (b)
was obtained from a powdered sample using a Rigaku Ultima IV X-ray
diffractometer. ..................................................................................................... 75
Figure 23. Powder X-Ray diffractogram of N,N,N’,N’-tetramethylethylenediammonium
succinate succinic acid. The simulated diffractogram (a) was obtained using the
Mercury version 3.5.1 software provided by the CCDC. The experimental
diffractogram (b) was obtained from a powdered sample using a Rigaku Ultima
IV X-ray diffractometer. ..................................................................................... 76
Figure 24. 13C CP/MAS spectra of sarcosine (top) and sarcosinium tartrate (bottom).
Spinning sidebands are denoted with asterisks. 𝐵0 = 9.4 T. ............................... 77
Figure 25. Selected regions of experimental 13C cross-polarization magic-angle spinning
(CP/MAS) NMR spectra of the methyl carbon associated with a tetrel bond. 𝐵0 =
9.4 T. (a) Sarcosinium Tartrate. (b) Sarcosine. ................................................... 78
IX
Figure 26. 13C CP/MAS spectra of N,N,N’,N’-tetramethylethylenediammonium dichloride
(top) and N,N,N’,N’-tetramethylethylenediammonium succinate succinic acid
(bottom). Spinning sidebands are denoted with asterisks. 𝐵0 = 9.4 T. ............... 79
Figure 27. Selected regions of experimental 13C cross-polarization magic-angle spinning
(CP/MAS) NMR spectra of the methyl carbon associated with a tetrel bond. 𝐵0 =
9.4 T. (a) N,N,N’,N’-tetramethylethylenediammonium dichloride. (b) N,N,N’,N’-
tetramethylethylenediammonium succinate succinic acid. ................................. 80
X
List of Tables
Table 1. Typical interaction strength of noncovalent interactions compared to some
examples of covalent bonds. A variety of examples were selected to present an
idea of expected interaction energy strengths. ...................................................... 7
Table 2. Functionals compared to QCISD in order to set a benchmark for determining the
highest performing functional as it applies to carbon tetrel bonding. ................. 55
Table 3. Computed values of the diamagnetic and paramagnetic contributions to the
magnetic shielding constants (d, p, and t) for the model structures. Values were
calculated by B3LYP and LC-PBE using the 6-311++G(d,p) basis set. .......... 65
Table 4. Computed chemical shift anisotropy data for model compounds using stated
functionals using the 6-311++g(d,p) basis set. .................................................... 67
Table 5. Calculated GIPAW and experimental 13C isotropic chemical shifts for the methyl
carbon on sarcosine compounds. ......................................................................... 81
Table 6. Raw data obtained from calculations (BHandHLYP/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz. ................ 103
Table 7. Raw data obtained from calculations (LC-PBE-D3/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz. ................ 106
Table 8. Raw data obtained from calculations (CAM-B3LYP/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz. ................ 109
Table 9. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(BHandHLYP/6-311++G(d,p)). ........................................................................ 111
XI
Table 10. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(LC-PBE-D3/6-311++G(d,p)). ....................................................................... 112
Table 11. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(CAM-B3LYP/6-311++G(d,p)). ....................................................................... 113
Table 12. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (MP2/6-311++G(d,p)). ........... 114
Table 13. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (B3LYP/6-311++G(d,p)). ...... 115
Table 14. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (LC-PBE/6-311++G(d,p)). .. 116
Table 15. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (LC-PBE-D3/6-311++G(d,p)).
........................................................................................................................... 117
Table 16. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (CAM-B3LYP/6-311++G(d,p)).
........................................................................................................................... 118
Table 17. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (BHandHLYP/6-311++G(d,p)).
........................................................................................................................... 119
XII
Table 18. CP -corrected energy and the 13C isotropic chemical shift vs the carbon tetrel bond
angle (CAM-B3LYP/6-311++G(d,p)). In all cases the angle was set so that the
oxygen or nitrogen was placed between two methyl hydrogen atoms. ............. 120
XIII
Abstract
Non-covalent bonds are an important class of intermolecular interactions, which
result in the ordering of atoms and molecules on the supramolecular scale. One such type of
interaction is brought about by the bond formation between a region of positive electrostatic
potential (-hole) interacts and a Lewis base. Previously, the halogen bond has been
extensively studied as an example of a -hole interaction, where the halogen atom acts as
the bond donor. Similarly, carbon, and the other tetrel elements can participate in -hole
bonds. This thesis explores the nature of the carbon tetrel bond through the use of
computational chemistry and solid state nuclear magnetic resonance (NMR) spectroscopy.
The results of calculations of interaction energies and NMR parameters are reported
for a series of model compounds exhibiting tetrel bonding from a methyl carbon to the
oxygen and nitrogen atoms in a range of functional groups. The 13C chemical shift (iso) and
the 1cJ(13C,17O/15N) coupling across the tetrel bond are recorded as a function of geometry.
The sensitivity of the NMR parameters to the non-covalent interaction is demonstrated via
an increase in iso and in |1cJ(13C,17O/15N)| as the tetrel bond strengthens. There is no direct
correlation between the NMR trends and the interaction energy curves; the energy minimum
does not appear to correspond to a maximum or minimum chemical shift or J-coupling value.
Gauge-including projector-augmented wave density functional theory (DFT)
calculations of iso are reported for crystals which exhibit tetrel bonding in the solid state.
Experimental iso values for sarcosine, betaine and caffeine and their tetrel-bonded salts
generally corroborate the computational findings. This work offers new insights into tetrel
XIV
bonding and facilitates the incorporation of tetrel bonds as restraints in NMR
crystallographic structure refinement.
XV
Acknowledgements
This work would not have been possible without the help and support of many
friends, family, colleagues and mentors that I’ve worked with over the past couple years.
First and foremost, I would like to thank Professor David L. Bryce, my supervisor, for his
exceptional guidance throughout my time in the Bryce Lab. Thank you for having confidence
in me, and providing me with a rich environment in which I could learn and excel. I look
forward to continuing working with you in the coming years. I would also like to
acknowledge Professors Alain St-Amant and Natalie Goto for reading this thesis and
providing to me valuable comments.
To my friends and colleagues at the University of Ottawa – thank you for your
support and your thoughtful discussions. Dr. Glenn Facey and Dr. Eric Ye at the University
of Ottawa NMR lab, your advice and technical support was invaluable throughout this work.
To my fellow Bryce Lab colleagues, I appreciate our collaboration over the years. Dr. Fred
A. Perras, you first introduced me to solid-state NMR on one of my first days in the lab. I
remember you making me spin up the DOR rotor that day without me knowing anything
about DOR at the time. Nothing could get me more interested in this field on the first day
than getting hands on work. Dr. Kevin M. N. Burgess, while we didn’t work together directly
that much, you taught me to value sober second thought when it came to the more
philosophical aspects of life. Dr. Jasmine Viger-Gravel, you taught me the importance of
being precise and meticulous in my research, a trait you’ve already perfected. To Pat Szell
and Sherif Nour, and more recent fellow graduate students Yijue Xu, Angel Wong, and Peter
Werhun, life in the office and in the lab wouldn’t be as interesting without you. Finally, a
XVI
special thank you needs to be made to Dr. Libor Kobera, who has gone above and beyond in
ensuring I am well trained in the finer aspects of NMR spectroscopy. I would finally also
like to take the opportunity to thank the various undergraduate students who I’ve also worked
with. Jeremy Chin, Michael West and Dylan Errulat, your hard work has produced quality
results.
Of course, all my time couldn’t be spent in the lab alone. I would like to thank my
friends and colleagues in my extended Canadian Armed Forces family for providing me with
an environment in which I could have fun and focus my mind on other things for a while.
Thanks to all of my mentors and supervisors: Maj. Jonathan McAuley, Capt. Dan Parker, the
team at OpsAir, and others whom I’ve worked for directly, for providing me with valuable
mentorship in challenging environments over the years. I believe that today I am a better
leader and your training and support has benefitted me greatly in my civilian life. Thank you
to my colleagues working in support of the Royal Canadian Air Cadets Program for all the
good times; in particular Lt. Alex Schmid, for keeping sane and motivated over the years.
It’s nice to be able to let off steam and vent once in a while! Unfortunately, there are too
many more to mention by name, but you all work so hard in providing an important and
valuable experience for Canadian youth and I’m grateful for your lasting friendships.
Finally, I would like to thank all of my family and relatives for their love and support.
Mom and Dad, over the years you’ve challenged me to go as far as I can in my education,
and you’ve ensured that I could realize my goals without too much trouble. Evan, you’ll have
to deal with that a little longer, but thanks for reminding me not to take anything for granted.
Thank you, Grandpa, in particular for always believing in me, and making me feel like a
“smart cookie”. Jane and Doug, thanks for being family to me when mine was so far away.
XVII
And finally, Alison, you’ve stood by me for everything, and I couldn’t imagine being with
anyone else as I move on to the next chapter of my life. You are the love of my life.
XVIII
“I have been looking for
someone to come up with NMR investigations on this interaction,
though, I thought it would be difficult. NMR evidence for hydrogen
bonding came nearly a century later. Tetrel carbon bonding
is barely a few years old.”
Elangannan Arunan
XIX
Statement of Originality
I certify that the work presented in this thesis is my own. With permission from the
publisher, the scientific contribution of this work is based on my own published work in a
peer reviewed journal. Sections 1.4 and 1.5, as well as Chapters 2, 3 and 4 are in part, or
wholly based on the work published in:
Southern, S. A. and Bryce, D. L. NMR Investigations of Noncovalent Carbon Tetrel Bonds.
Computational Assessment and Initial Experimental Observation. The Journal of Physical
Chemistry A, 2015, 119, 11891-11899. DOI: 10.1021/acs.jpca.5b10848.
Chapter 1 – Introduction
1
Chapter 1 - Introduction
1.1 The Basic Properties of Matter
It has been a long time since the idea of the particle first emerged among humans.
The imaginations of the ancient Greek philosophers led them to believe that matter was
not simply made of what could be seen, but rather individual units. Plato first suggested
that matter was essentially divided into polyhedral subunits called elements: earth, air,
water and fire. From that point, the great philosophers argued whether matter was
continuous, or made from discrete units, trying for many years to resolve the issue before
them.
The quest for the answer was later resolved by John Dalton, who first proposed
the idea of atomic theory.1,2 Since then, science has evolved to the point now, where
matter has been almost fully characterized right down to the subatomic level, so far as
even observing the elusive Higg’s boson.3,4
In this tiny world, particles behave much differently than one would expect.
Humans are used to seeing that when a baseball is thrown by the outfielder, it forms an
arc before it arrives at the baseman; this motion is a result of classical mechanics.
However, we must use quantum mechanics to describe the intricate details of the nature
of the subatomic particles; the constituents of the atom.
Atoms are particles which are composed of electrons, neutrons and protons. When
atoms are combined together, they form matter, which can form materials that we are
more familiar with and that we can interact with. The atom can be described as a nucleus
containing the neutrons and protons, surrounded by the orbiting electrons (Figure 1).
Chapter 1 – Introduction
2
Figure 1. A basic representation of a 12C atom using the Rutherford-Bohr model. The
nucleus (blue) is surrounded by the orbit of electrons occupying two energy levels. Two
electrons (yellow) reside in the n=1 shell, and four in the n=2 shell. Note that further
electronic orbitals may exist beyond those that are occupied in the case of an excited
electronic state.
The atom is defined by its atomic number, which represents the number of protons
residing within the nucleus. The atomic weight is the average of all the weights of each
isotope, weighted according to their abundance in nature. An isotope of a particular
element is one which has a different number of neutrons than the other.5 For example,
while 12C contains six neutrons and six protons, 13C contains seven neutrons, and six
protons. A given atom that is isolated will always carry the same number of electrons,
regardless of the isotope.
The electron configuration of a particular atom describes the arrangements of its
electrons in terms of discrete atomic orbitals. It assumes that only two electrons may
Chapter 1 – Introduction
3
occupy a given atomic orbital, as defined by the Pauli Exclusion Principle.6,7 Closest to
the nucleus is the 1s-orbital. Further away are the p-, d-, and f-orbitals, each with x, y, and
z Cartesian components. Consider a 12C atom, which has six electrons. Its formal
configuration is 1s22s22p2 because it has two electrons in its core orbital, and a total of
four electrons in the valence s- and p-orbitals. It is worth noting that in quantum
mechanics, the square of the atomic orbitals represent the probability of observing
electron density at any point in space surrounding a nucleus, so they exist in various
shapes and symmetries. 7 The larger the atom, the more electrons it has, and therefore the
more orbitals that are filled. Hund’s rule8,9 states that the electronic orbitals are filled with
one electron, before filling it with a second. So when there are three p-orbitals of the same
energy, each must be filled by one electron before they can be filled again by a second
electron. To illustrate this, Figure 2 shows the electronic configuration of fluorine, where
the 2𝑝-orbitals are each filled by one electron, then by a second electron of opposing spin.
The 2𝑝𝑍-orbital remains filled with only one electron.
Chapter 1 – Introduction
4
Figure 2. The electronic configuration diagram for a single fluorine atom (1s22s22p5).
The filling of the molecular orbitals, with increasing energy, follows Hund’s rule.
In describing the electronic orbitals as a set of allowed states which the electrons
can possess, they can be quantized by the quantum number, n. By doing this, the idea of
quantum mechanics is introduced to the description of the atom. Quantum mechanics is
the more accurate description and it will be used throughout this thesis.
Protons have a net positive charge, and electrons hold negative charge. However,
this is a simplistic view of the particle, and in fact, their character becomes more complex.
In fact, the description of subatomic particles may include such characteristics as spin,
angular momentum, and magnetic moment.
Nuclear spin is an important property of the nucleus. Just as the Earth rotates
around its axis, spin can be thought of, in a classical sense, as the rotation of a nucleus
around its own axis.10 Consequently, particles possess spin angular momentum. Consider
a gyroscope. When it is spun, it tends to remain in place until a force is acted upon it due
Chapter 1 – Introduction
5
to the conservation of angular momentum. While it may seem quite familiar, this classical
description of the elementary particle is, of course, false, and indeed nuclei do not actually
rotate around axes in the way a planet does. Instead, chemists resort to quantum
mechanics in order to properly describe the angular momentum due to the fact that
subatomic particles display properties of both particles and waves (the wave-particle
duality). Spin is an intrinsic property10, and it may be described as α or β; being “up” or
“down,” respectively. They are represented in the electronic configuration diagrams by
upward and downward arrows, respectively (Figure 2).
1.2 Noncovalent interactions
Noncovalent interactions are the result of the interactions between electrons
resulting from their charge distributions over a particular atom or molecule. These
interactions can, consequently, exist between two different molecules or within a
molecule but between nearby groups. Some examples of noncovalent interactions include
van der Waals (vdW) interactions, 𝜋-interactions and electrostatic interactions.
Electrostatic interactions, such as the dipole-dipole interaction is an example of
an attractive vdW interaction arising due to the electronic dipoles formed from the
asymmetric distribution of electrons over the surface of an atom or a molecule, where
some regions tend to be more electronegative than others.5 In some cases, that region may
also possess a formal charge. For example, two molecules of acetone may interact
between the carbonyl oxygen of one molecule and the carbonyl carbon of the other.
Hydrogen bonds exhibit partially noncovalent character (Figure 3), whereby the partially
Chapter 1 – Introduction
6
positive charge on the hydrogen atoms can interact with a partially negative charge.11,12
𝜋-interactions may, for example, occur between the negative charge distribution on
aromatic faces resulting from the 𝜋-orbitals, and any partially positive or formally
positive counter charge, such as an ion or another aromatic ring. These interactions are
quite weak, on the order of less than 10 kcal/mol, yet significant especially in protein
folding or molecular signalling, because amino acids histidine, tryptophan,
phenylalanine, and tyrosine all contain aromatic rings with 𝜋-systems.13,14
Figure 3. The hydrogen bond. The electrostatic interactions between the partially positive
(δ+) and partially negative (δ-) charge contribute to an attractive interaction between the
oxygen and hydrogen atoms in water molecules.
Noncovalent bonding mediated by -holes has been studied extensively in the
context of halogen bonding15,23,24, pnicogen bonding 16,17, chalcogen bonding. 18,19,20,21
Bonding involving the noble gases, coined “aerogen bonding”, has also been explored in
the recent years. 22 Halogen bonding23,24 is an example of a noncovalent interaction, where
Chapter 1 – Introduction
7
an area of partially positive charge, called a 𝜎-hole25,26, acts as an electrophile for a
negatively charged or electron rich molecule.
Each of the preceding are examples of hole interactions which is a subclass of
noncovalent interactions.27,28 In every case, the bond donors interact with a Lewis base
like entity, such as electronegative atoms or lone pairs of electrons (Figure 5). As with
covalent bonds, the strength of the hole bond can be expressed in terms of energy,
whereby the resulting energy is known as the bonding energy.
Table 1. Typical interaction strength of noncovalent interactions compared to some
examples of covalent bonds. A variety of examples were selected to present an idea of
expected interaction energy strengths.
Interaction
Interaction Strength
/ kcal mol-1
Covalent Bond C-C 8529
C-H 10029
C=O 17529
Hydrogen Bond 1-329
PHN 0.830
van der Waals Interactions 0.5-129
Halogen Bond 1-731
chloro-cyanoacetylene 2.332
Chalcogen Bond H2SCl- 0.8133
SCSCl- 10.5933
F4SNH3 1421
Pnicogen Bond FNN 430
PNN 730
F4PNH3 4317
H3FPNH3 3617
Chapter 1 – Introduction
8
1.2.1 Sigma-Holes
Computational examination of the electrostatic potential (ESP) surfaces of
halogen bonding molecules revealed that on one side of the interaction, there was an area
in which different charges were present on a single atom.25,26
Consider a symmetric atom in a vacuum in the absence of any external effect of
charge, magnetism or other influences. In the case of this lone atom, the ESP is generally
positive because the effect of the nucleus dominates over the effect of the electrons which
are dispersed over the entire atom.34 The electrostatic potential resulting from the
contributions of the electron density, 𝜌(𝑟), and the charge on the nucleus, 𝑍𝐴, at any point
𝑟 on the surface of an atom is given by34:
𝑉(𝑟) = ∑𝑍𝐴
|𝑅𝐴 − 𝑟|− ∫
𝜌(𝑟′)𝑑𝑟′
|𝑟′ − 𝑟|𝐴
1
where the distance between the point and the nucleus is 𝑅𝐴. Typically, the 𝜌(𝑟) =
0.001 electrons/bohr3 surface is used to represent a molecular surface, corresponding to
an electrostatic potential of 𝑉𝑠(𝑟). When the effects of the electrons dominate at a given
point, the expression yields a negative value on the potential surface. The ESP provides
an effective and convenient way to model the σ-hole in noncovalent bonding.26
The σ-hole is an area at which 𝑉(𝑟) has a value that is more positive than the
surrounding area, thus indicating and area of electronic depletion. When the atom of
interest is covalently bound to another atom or functional group with electron
withdrawing character, such as a trifluoromethane group, a substituted aromatic ring, an
amino group, the tendency is for the electronic distribution to be drawn toward the
Chapter 1 – Introduction
9
covalent bond. This gives rise to a hole situated along the extension of the covalent
on the opposite side of the atom of interest. The point representing the hole can be
depicted as 𝑉𝑠,𝑚𝑎𝑥 because it typically portrays a local area of maximum electrostatic
depletion.15
The electrostatic depletion at 𝑉𝑠,𝑚𝑎𝑥 can be explained using natural bond order
(NBO) analysis.35 It has been shown that the halogen bond donor atoms tend to possess a
sigma bonding orbital as well as three unshared pairs of electrons, each occupying the p-
orbitals. The 𝑝𝑧 orbital lying along the axis of the covalent bond is half filled, resulting
in an 𝑠2𝑝𝑥2𝑝𝑦
2𝑝𝑧1 character. The result is therefore a “belt”35 of negative electrostatic
potential around the halogen atom, leaving an area of electronic deficiency on the
opposite end of the covalent bond; the hole.26 The magnitude of this electronic
deficiency comes down to the amount of s character is present in the p-orbital; the more
purely p the orbital is, the stronger the hole.26 The hole can be effectively neutralized
by a negative group such lone pair of electrons, and this accounts for the high degree of
linearity in such an interaction.36 The situation is somewhat different with respect to the
group IV tetrel elements. The tetrel elements do not have lone pairs of electrons, and are
as such sp3 hybridized. Consequently, there is a large amount of s-character in the bonding
orbitals. The conclusion is, however, that reduced p-character of the bonding orbital is
acceptable, and the hole remains present, albeit weaker.36
Chapter 1 – Introduction
10
Figure 4. The electrostatic potential at the 0.001 a.u. surface of various structures
exhibiting σ-holes. The σ-hole is present on (b) chloromethane; (c) fluoromethane; (d) a
methyl group that is covalently bonded to methylammonium. For illustration purposes, a
molecule of methane (a) is shown and does not to possess a sigma hole on carbon. Instead,
the area where the hole ought to be is more negative due to the electronic depletion
over the hydrogen atoms (each of which coincidently possess a single hole15). The red
colour corresponds to electrostatic potential values ≤ 0.172 a.u. and the blue colour
corresponds to electrostatic potential values ≥ 0.179 a.u.
The strength of a σ-hole depends significantly on the electron withdrawing
character of its covalently bonded partner atom or molecule.36 Considering iodine, bound
to a methyl group, one is not likely to observe a significant hole. In this case, the methyl
carbon is not considered to be very polarizing because the hydrogen atoms do not have
any polarization capabilities. In fact, the polarization strength of iodine has a greater effect
and it would be more likely that a negative hole would be found on the iodine atom,
and a positive hole on the carbon. 26 Conversely, when fluorine atoms, or other
Chapter 1 – Introduction
11
electron-withdrawing substituents such as aromatic rings, are substituted for the hydrogen
atoms, a relatively strong hole is introduced as a result of the increased electron
withdrawing ability of the other group.26.19
The electronic potential of a number of holes generated by various electron
withdrawing substituents has been listed by Politzer et al.27 They show that the strongest
holes are achieved when cyanide groups are used, although these holes are achieved
only when the entire isoelectric surface is positive in nature. Other substituents, such as
fluorine and chlorine, also contribute to the formation of holes.15 in general, 𝑉𝑠,𝑚𝑎𝑥
becomes increasingly positive as the rest of the molecule becomes more electron-
withdrawing.37
1.2.2 Sigma Hole Bonding
Consider a molecule or fragment RX interacting with a nucleophilic molecule or
fragment Y (often an anion, a Lewis base, or -electrons). The -hole is on X along the
extension of the covalent bond to R (Figure 5). Depending on the identity of element X,
such interactions take on their own names in the literature, e.g., halogen bonding,
pnicogen bonding, chalcogen bonding, and aerogen bonding, where the name of the
interaction refers to the periodic table group to which the bond donor (electron acceptor)
belongs (group V: pnicogens; group VI: chalcogens, etc.).38 These are all different types
of -hole bonds.
Chapter 1 – Introduction
12
Figure 5. General schematic of a tetrel bond, where R is a covalently bonded atom or
functional group, X is the tetrel bond donor (X = C, Si, Ge, Sn, or Pb), and Y is the tetrel
bond acceptor.40 dX-Y is smaller than the sum of the van der Waals radii of the interacting
atoms.
The hole has been studied extensively as it applies to halogen bonding.
Considering again the iodine atom covalently bound in I-CF3, one would expect to
observe a relatively significant hole. In terms of its electropositive character, the
magnitude of 𝑉𝑠,𝑚𝑎𝑥 within the hole increases as the atomic number of the halogen
increases, thereby increasing the interaction strength of the halogen bond.15 For example,
the hole bond between a -electron and an iodine atom would be greater than that
resulting from a bromine atom.
In general, the bonding energy is a negative value, representing an attractive
interaction. The correlation between the 𝑉𝑠,𝑚𝑎𝑥 and the interaction energy is such that
when the electronic depletion on the hole is increased, the magnitude of the bond
strength increases as well. It can therefore be expected that bond donors with higher
atomic numbers will more readily form bonding interactions. That’s not to say that
Chapter 1 – Introduction
13
weakly polarized atoms such as carbon will not participate in these types of bonds; the
bonds will simply be weaker in nature and sometimes difficult to produce by
crystallization.
1.3 Group IV “Tetrel” Bonding
The focus of this thesis is on tetrel bonding, named after the bond donor, which falls under
group IV in the periodic table.36,39,40,56 In an R-C···Y carbon tetrel bond (Figure 5), the
-hole resides on carbon. As noted by Politzer27, often in such group IV cases, all or
almost all of the electrostatic potential on the R-C moiety is positive and in such cases the
-hole is simply identified as a region which is more positive than its surroundings
(Figure 4), leading to the preferential formation of an interaction from the -hole over
other types of complexes.
As is generally the case for -hole bonds, the strength of the tetrel bond depends
largely on the atomic number of X and by the electron withdrawing ability of the R
substituents.41,42,43 The nature of the tetrel bond donor has an impact on the tetrel bond
strength, whereas the atomic size of the bond donor increases from C to Sn, the bonding
energy increases. This is attributed to an increase in the polarizability of the atom as one
goes down the periodic table, thus increases the size of the hole.
Chapter 1 – Introduction
14
Figure 6. (a) The electrostatic potential at the 0.001 au surface of positively charged
dimethylammonium (left) and formaldehyde (centre) computed by CAM-B3LYP/6-
311++G(d,p). The red colour on dimethylammonium (right) corresponds to electrostatic
potential values ≤ 0.172 au; the blue colour corresponds to electrostatic potential values
≥ 0.179 au. The -hole is present on the methyl carbon and is adjacent to the C-N -bond,
and it has an electrostatic potential value of 0.179 au. (b) A carbon tetrel bond involving
a methyl carbon. (c) An example of a carbon tetrel bond occurring in the crystal structure
of sarcosinium tartrate.44
Experimental evidence for tetrel bonding involving Si and Sn has been in the
literature for many years. Silicon tetrel bonding was noted to mediate chemical reactions
by its hexacoordinated intermediate.45 In other cases, hexacoordinated tetrel bonded
silicon atoms have been observed to exist in various species. 46,47 Inter- and
intramolecular tetrel bonding of silicon and lead atoms have also been demonstrated
through crystallographic methods.48,49,50
Chapter 1 – Introduction
15
Additional evidence for the existence of tetrel bonding involving carbon as well
as silicon has been growing significantly in recent years.36,39,51,52 Quantum calculations
have confirmed the presence of carbon tetrel bonds between electron deficient carbon
atoms and electron rich tetrel bond acceptors.40,42,53,54 The importance of the tetrel bond
may be analogous to other forms of noncovalent bonding. Given that carbon atoms are in
abundance in nature and in synthetic chemistry, carbon tetrel bonding may play important
roles in the organization of molecular units, from natural products to functional materials
and pharmaceuticals. Furthermore, it could be envisaged that carbon tetrel bonding could
play a role in directing molecular orientation in some dynamic systems, such as protein
folding, ligand-acceptor interactions, or other processes of biological importance.40,55 For
instance, it has recently been suggested that the carbon tetrel bond could play a critical
role in directing SN2 reactions (Figure 7).56 A search of the Crystal Structure Database
(CSD) demonstrates that there are perhaps thousands of examples where the tetrel bond
interactions exist, and could be contributing to the three-dimensional packing
arrangements of molecules within their crystal lattices.
Figure 7. A schematic showing the influence of a tetrel bond on the activation of an SN2
reaction. Inspired from the work of Grabowski.56 Purple: fluorine; Grey: carbon; White:
hydrogen; and Yellow: chlorine.
Chapter 1 – Introduction
16
Recently, Arunan related the atoms in molecules (AIM) descriptors for a hydrogen
bond57 to the carbon tetrel bond, an implication that similar rules could be applied to tetrel
bonding.15 These criteria are meant to test for the presence of a bond path indicative of a
noncovalent interaction (a hydrogen bond in the original paper). Among these criteria
were: 1. A bond path linking two interacting atoms must connect the bond critical point
which is present between both atoms; 2. There must be mutual penetration of the electron
density clouds; 3. On the formation of the complex, the bond donor loses some charge,
and there is some destabilization on the donor atom; 4. The atomic volume of the donor
atom decreases. In almost all of the examples presented by Arunan, the carbon tetrel
bonded complexes follow the proposed behaviour of hydrogen bonds.
IR spectroscopic studies on tetrel bonded complexes have shown that there is a
red shift in the C-X stretching frequency due to hyperconjugation of lone pair orbitals of
the bond acceptor and the anti-bonding orbital of the bond donor.15 This causes a
weakening of the sigma bond between X and C causing a decrease in the stretching
frequency.
Finally, computational work in 2009 provided key evidence predicting -hole
bonding to the lightest tetrel element, carbon.36 More recently, Thomas et al. identified
716 compounds which may exhibit C···O tetrel bonding in the compounds in the CSD.58
They conducted important experiments providing charge density analysis of fenobam and
dimethylammonium 4-hydroxybenzoic acid in the solid state, each exhibiting carbon
tetrel bonds. The results indicated the presence of a tetrel bond on the latter structure.
Chapter 1 – Introduction
17
However, the former preferentially formed hydrogen bonds between the methyl hydrogen
and the associated chlorine atom.
1.4 Nuclear Magnetic Resonance Spectroscopy
1.4.1 The Zeeman Interaction
It is useful to begin the discussion of nuclear magnetic resonance (NMR) by first
discussing the basics of quantum mechanics. Nuclei possess a nuclear spin quantum
number, 𝐼, which can take the values of integers and half integers of 0, ½, 1, etc.,
increasing in intervals of one half. Nuclei possessing spin with integer values of 𝐼 are
known as bosons while nuclei with half-integer spin values are called fermions.10
Related to spin is the property called angular momentum, 𝐿, given by eqn. 2 as:10
𝐿 = ℏ√𝐼(𝐼 + 1) 2
The nuclear spin angular momentum is a vector with a component along the z-axis. The
z-component interacts directly with the applied magnetic field, 𝐵0 (reported in units of
Tesla (T)), which also lies along the z-axis. It is for this reason that the angular momentum
operator representing its z-component can therefore be defined by 𝐼𝑧.
The angular momentum gives rise to an intrinsic property called magnetic
moment, 𝜇, representing the interaction between the nucleus and the magnetic field.10 𝜇
is dependent on both the nuclear spin angular momentum and the gyromagnetic ratio, 𝛾
(rad s-1 T-1). The total energy from this interaction is given by:59
Chapter 1 – Introduction
18
𝐸 = −𝜇𝐵0 3
The spin quantum number, 𝐼, has corresponding eigenvalues of 𝑚𝑙, equal to – 𝐼 to
+𝐼 in intervals of 1. Thus, for any value of 𝐼, there are precisely (2𝐼 + 1) eigenvalues.
The 𝐼𝑧 operator has (2𝐼 + 1) eigenfunctions. In general, this can be represented by:
𝐼𝑧𝜓𝑚 = 𝑚𝑙ℏ𝜓𝑚 4
It is now useful to define the Hamiltonian for a spin in a magnetic field. The
Hamiltonian operator is dependent on the gyromagnetic ratio, 𝐵0, and the angular
momentum operator. Eqn. 5 describes the Hamiltonian:
�̂� = −𝛾𝐵0𝐼𝑧 5
Thus, when the Schrödinger equation for a single spin in the magnetic field is
given by:
�̂�𝜓𝑚 = 𝐸𝑚𝜓𝑚 6
where the energy, 𝐸𝑚 (in units of Joules) representing the eigenstates of the nuclear spin
in the presence of the magnetic field is given by eqn. 7:
𝐸 = −𝑚𝑙ℏ𝛾𝐵0 7
Each energy state can be labelled as an α state or a β state, representing the lower
energy and higher energy levels, respectively. These eigenstates are related to the
Chapter 1 – Introduction
19
magnetic moment such that lowest possible energy is brought about by perfect alignment
with the magnetic field. The transition energy corresponds to the energy which must be
subjected to a nuclear spin in order to induce a transition from the α state to the
corresponding β state, matching to a specific electromagnetic frequency. This is referred
to as the NMR transition, and the transition can only occur when the difference between
both values of 𝑚𝑙 is equal to exactly one. The frequency of the photon that will induce an
NMR transition, or the Zeeman Effect (Figure 8), is given in eqn. 8, where 𝜈0 is the
Larmor frequency, and is isotopically specific due to its dependence on the gyromagnetic
ratio.
𝜈0 =𝛾𝐵0
2𝜋 8
In a simple system, one would expect a line on the NMR spectrum at the exact
frequency of 𝜈0. However, this is not typically the case because nuclear spins are usually
affected by their chemical environments. The energy eigenvalue becomes significantly
more complex as the nature of the nearby electrons, as well as the coupling to other nuclei
is taken into account.
Chapter 1 – Introduction
20
Figure 8. The Zeeman Effect for a spin 1
2 nuclide. The splitting of the spin states is
observed as a function of the strength of the magnetic field.
In the absence of a magnetic field, the direction of the spins is isotropic.10 When
a sample is placed in 𝐵0, the interaction of the spin nuclear magnetic moments with the
magnetic field will cause their bulk alignment with 𝐵0. This is a process that is time
dependent and is known as 𝑇1 spin-lattice relaxation. The net equilibrium magnetization
can be represented by the vector, �⃑⃑⃑� . In the end, the spin polarization does not align with
the magnetic field per se, but instead, the magnetic moments cause the spins to rotate
around 𝐵0 in the shape of a “precession cone”10 with oscillations equal to 𝜈0. The z-
component of the magnetization is important for NMR.
At the thermal equilibrium, the distribution of spins in the high energy state versus
the low energy state is governed by the Boltzmann distribution:
Chapter 1 – Introduction
21
𝑛𝛼2
𝑛𝛽1= 𝑒−
Δ𝐸𝑘𝑇 9
The NMR experiment is therefore the practice of manipulating the magnetization
vector through space. A sample is placed in a coil which is situated in the xy-plane
perpendicular to 𝐵0. By applying a radiofrequency (RF) pulse along the x- or y- axis, the
magnetization may be tilted away from the z-axis. In doing so, the magnetization
precesses around the z-axis at the Larmor frequency, resulting in a component of the
vector oscillating in the xy plane. The vector oscillations can be detected as it induces a
current in the coil. These oscillations are detected by the spectrometer. The magnetization
vector continues to precess around the z-axis, but the cone eventually returns to the
thermal equilibrium along the z-axis, causing a gradual decrease of the xy component of
the magnetization over time. The detected current in the coil resulting from the
oscillations in the xy-plane is known as the free induction decay (FID). The FID is
transformed from the time domain to the frequency domain through Fourier transform to
an NMR spectrum.
As it was mentioned before, nuclear spins are affected by their chemical
environments. For example, the effects of the electrons shielding the interaction between
the nucleus and 𝐵0 would have a direct effect on the resulting NMR transition. Other
effects, such as spin-spin coupling, or the quadrupolar interaction of some nuclides can
have a major impact on the NMR spectrum. These NMR interactions are essentially
perturbations to the Zeeman interaction. Thus, the NMR spectrum is complicated by the
fact that these interactions exist.
Chapter 1 – Introduction
22
The Hamiltonian for a spin in a magnetic field is therefore not only dependent on
the Zeeman Hamiltonian alone (eqn. 5). In fact, it is additionally dependent on the
magnetic shielding interaction, the direct and indirect dipolar coupling interactions, and
the quadrupolar interaction in the case of nuclides with spin greater than 1
2. It is therefore
essential to examine some of these interactions in detail. For the purposes of this thesis,
only the magnetic shielding interaction as well as the indirect spin-spin J-coupling
interactions will be discussed in detail.
1.4.2 Magnetic Shielding
Magnetic shielding is brought about by the magnetic fields generated by the
electrons. These fields may be additive or subtractive to 𝐵0, and consequently change the
way the nuclear magnetic moment interacts with the magnetic field. The magnetic field
seen by the nucleus as a result of the effects of magnetic shielding is given by:
𝐵𝜎 = (1 − 𝜎)𝐵0 10
where 𝜎 is the shielding constant.
Using the secular approximation, the magnetic shielding operator is shown in eqn.
11 to be dependent on the gyromagnetic ratio and the shielding constant.
�̂�𝜎 = −𝛾ℏ𝜎𝐵0𝐼𝑍 11
Chapter 1 – Introduction
23
The magnetic shielding interaction is anisotropic by nature, meaning it is
orientationally dependent. In expression 12, the magnetic shielding tensor is diagonalized
such that the interaction is represented by its principal axis system (PAS).
[
𝜎𝑥𝑥 𝜎𝑥𝑦 𝜎𝑥𝑧
𝜎𝑦𝑥 𝜎𝑦𝑦 𝜎𝑦𝑧
𝜎𝑧𝑥 𝜎𝑧𝑦 𝜎𝑧𝑧
] ⇒ [
𝜎11 0 00 𝜎22 00 0 𝜎33
] , 𝜎11 ≤ 𝜎22 ≤ 𝜎33 12
The isotropic shielding constant, 𝜎𝑖𝑠𝑜, is given as the average of the three shielding
tensor components (eqn. 13). Further parameters which may be used are the span, Ω, and
the skew, κ, measuring the breadth of the signal and the asymmetry, respectively (eqn. 14
and 15).60 The span is related to the distribution of the signals corresponding to the
orientations the molecule takes in the sample, which is averaged out in a solution, and the
skew is the asymmetry of the distribution of the signals.
𝜎𝑖𝑠𝑜 =𝜎11 + 𝜎22 + 𝜎33
3 13
Ω = 𝜎33 − 𝜎11 14
κ =3(𝜎𝑖𝑠𝑜 − 𝜎22)
Ω
15
The shielding constant is observed directly in the NMR spectrum in the form of a
chemical shift. The chemical shift is the value of 𝜎 with respect to a reference. For
example, the secondary reference for a 13C spectrum could be glycine, and the chemical
shift of the carbonyl carbon is 176.4 ppm with respect to tetramethylsilane (𝛿𝑖𝑠𝑜TMS =
0 ppm).61 In units of Hz, the chemical shift is defined by eqn. 16:
Chapter 1 – Introduction
24
𝛿 =𝜎𝑟𝑒𝑓 − 𝜎
1 − 𝜎𝑟𝑒𝑓 16
The preceding formula can also give the chemical shift in units of parts per million
by simply multiplying by 106.
1.4.3 Spin-spin coupling
In general, coupling results from the interaction between two different spins.
Indirect spin-orbit coupling (J-coupling) occurs when the interaction between two nuclear
spins is mediated by the electrons involved in their bonding.
J-coupling is typically only a very small perturbation to the Zeeman interaction.
Therefore, it is likely that the other NMR interactions overshadow the presence of this
interaction because it tends to be on the order of a few Hz for first-row elements.
Nevertheless, J-coupling is a very important tool for probing the connectivity of atoms in
a molecule.62 In units of Hz, the J-coupling operator between nucleus 1 and 2 is:
�̂� = 2𝜋𝐼1𝐽𝐼2 17
In the preceding Hamiltonian, 𝐽 is the orientation-dependent J-coupling tensor.
The isotropic J-coupling (𝐽𝑖𝑠𝑜) is the average of the principal components of the tensor.
The anisotropic contribution to J-coupling (Δ𝐽) is averaged out in the molecular tumbling
of an isotropic solution. However, in the solid state, it remains present, albeit often small.
The sign of 𝐽𝑖𝑠𝑜 is dependent on the gyromagnetic ratios of each of the spins for the case
of single bonds.
Chapter 1 – Introduction
25
Ramsey’s theory63 states that there are precisely five mechanisms that contribute
to the total J-coupling. Fermi contact (FC) is typically the dominant contribution to J-
coupling. It is important to recall that s-orbitals have electron density at the nucleus. The
FC contribution arises due to the interaction of the electronic spins and the nuclear spins
when the electronic density is at the nucleus. Therefore, the FC contribution is typically
a good indicator of chemical bonding. The paramagnetic spin orbit (PSO) and the
diamagnetic spin orbital (DSO) mechanisms emerge due to the coupling of angular
momenta of the electrons around two nuclear spins. The spin dipole (SD) term is simply
due to the coupling between the nuclear and the electronic spins. Finally, there exists a
(FC × SD) cross term which is usually a major contribution Δ𝐽. It is important to note that
the FC mechanism does not contribute to Δ𝐽.64
1.4.4 Other NMR interactions
Other contributions to the total nuclear spin Hamiltonian which arise due to the
interaction with a magnetic field are dipolar coupling and quadrupolar coupling. Direct
dipolar coupling is a case of nuclear spin coupling, but in this case it is a result of the
interaction of the two magnetic dipoles resulting from the magnetic moments of each of
the nuclei. It is a through space interaction, as opposed to J-coupling, which is a through-
bond interaction mediated by interceding electrons. Accordingly, dipolar coupling can be
used to measure the distance between nuclei or give global snapshots of macromolecules.
65,66
Chapter 1 – Introduction
26
The quadrupolar interaction affects nuclei that have spin greater than 1
2.10 The
quadrupolar interaction arises because these nuclei have a non-spherical distribution of
charge within the nucleus. This distribution is expressed as the quadrupole moment, 𝑄,
which couples with the electric field gradient (EFG) caused by the nuclei and electrons
within the molecule. This interaction is often very strong, so the quadrupolar interaction
usually dominates the NMR spectra of quadrupolar nuclides.
Using all of the preceding NMR interactions, it possible to obtain a substantial
amount of information about the electronic structure of a molecule. This is the power of
solid-state NMR spectroscopy; it is a tool that has the potential to reveal a lot of
information that can lead to conclusions about the nature of molecular systems. In this
work, solid state NMR is used to reveal the nature of noncovalent chemical bonding
between atoms.
1.5 Objectives
It is clear that noncovalent bonds play important roles in every aspect of life and
chemistry. It is therefore extremely important to fully understand how they work so as to
develop more efficient strategies for dealing with the molecular chemistry and properties
of materials.
Previously, there has been only limited analysis of -hole bonds involving the
Group IV “tetrel” elements. Tetrel bonds with carbon acting as the bond donor are
considered to be of great importance since carbon atoms are greatly abundant in nature
Chapter 1 – Introduction
27
and in chemistry. Therefore, further research into the area of tetrel bonding is extremely
important.
Nuclear magnetic resonance (NMR) spectroscopy is an important tool for
furthering the understanding of noncovalent interactions. Work on halogen bonds, using
both experimental and computational methods, has demonstrated the sensitivities of
chemical shifts, quadrupolar couplings, and J-couplings to the halogen bond geometry in
crystalline materials.67,68,69,70,71 In methyl tetrel bonds, it has been shown that the methyl
hydrogens surrounding the tetrel bond experience a decrease in their chemical shifts.72
The major goal of this thesis is to determine whether the presence or the absence
of a tetrel bond can be detected using solid-state NMR. In the present study, investigations
into carbon tetrel bonding are expanded using NMR quantum chemical calculations and
solid-state NMR spectroscopy with the goal of observing how the presence of carbon
tetrel bonds, and their geometries, may affect the NMR response. The NMR parameters
observed are chemical shifts, providing an indication of the magnetic shielding on the
tetrel atom, and the computed J-coupling, giving insights to the connectivity of the tetrel
bond.
Chapter 2 – Instrumentation and Methodology
28
Chapter 2 - Instrumentation and Methodology
2.1 Sample Preparation
2.1.1 Introduction to Theoretical Aspects of Powder X-Ray Diffraction
The work of this thesis was complemented by an analytical technique known as
powder X-ray diffraction (PXRD). Specifically, the identities of the synthesized crystals
were confirmed by PXRD as it allows for crystal structural determination using powdered
samples. In comparison to single crystal X-ray diffraction, PXRD can be more efficient as it
avoids the need for growing single crystals, which can be a long, sometimes laborious, and
often costly endeavour.
It has certainly been possible, while not very trivial, to solve ab initio a crystal
structure using PXRD.73,74,75 In this work, rather than solving the crystal structure, PXRD
results are compared to known data to verify the correct product has been produced.
In PXRD, the sample is bombarded with X-rays from angles set by the user. The
range of angles depends entirely on the sample since the signals generated from the X-ray
diffraction on the diffractogram are obtained as a function of the angle. In many cases, no
diffraction pattern past the angle of 65 degrees may be obtained, while with other samples,
the range may be larger or smaller. The peaks in the diffractogram depend ultimately on the
crystal structure of the compound.
First, the sample is spread onto a sample plate made of either glass or some metal. It
is then placed in the X-ray diffractometer, which consists of a cathode ray tube that generates
X-rays. The resulting X-rays are passed through a monochromator in order to filter out
unwanted wavelengths of electromagnetic radiation. The X-rays then make contact with the
Chapter 2 – Instrumentation and Methodology
29
surface of the material, and are either scattered by the atoms in the sample, or passed to the
next layer of atoms to either scatter or pass through again. Constructive interference occurs
when the X-ray beams from two different layers are in phase. This is detected and shown as
a peak on the diffractogram. This process follows Bragg’s Law:
𝑛𝜆 = 2𝑑 sin 𝜃 18
where 𝜆 is the wavelength, 𝑑 is the spacing between the layers, and 𝜃 is the incident angle
of the X-ray beam. The detector accepts the X-rays at an angle of 2𝜃 from the cathode ray
tube as both rotate around the sample, and the diffraction pattern is hence reported as a
function of 2𝜃 on the diffractogram. This is known as the Bragg-Brentano method.
2.2 Quantum Computational Chemistry
2.2.1 The Hartree-Fock Method and the Self Consistent Field
Quantum computational methods allow chemists to study complex systems existing
with more than one electron in order to understand its fundamental properties. Ab initio
methods have enabled the calculation of the electronic information of complicated systems,
which gives researchers better insights into the intricate details of their study. In many fields,
quantum computational methods allow for the de novo discovery of the properties of various
materials which cannot be studied alternatively. However, in this work, quantum chemical
computing is used as a means to complement the findings of experimental studies in order to
achieve a greater confidence to the solution of a given problem.
Chapter 2 – Instrumentation and Methodology
30
In order to successfully employ quantum chemistry, it is important to properly
understand the basics of how it works. It is often the case that a person will use a tool at their
disposal but it is not always that the user knows how that tool works. In order to fully
appreciate the power of quantum computational chemistry, the fundamentals aspects must
be understood.
The electronic structure of a system can be described by the solution to the time
independent Schrödinger equation. The solution to the Schrödinger equation can be entirely
independent of any experimental information, making it a first principles method. Solving
the electronic structure is, however, a very difficult task. Except for the case of a single, and
sometimes even a dual electron system, it is not computationally feasible to obtain the exact
solution. Ab initio methods usually always employ some sort of technique to solving the
Schrödinger equation through various simplifications and approximations, and therefore
allow for very close estimations of the true solution, but not necessarily the solution itself.
The time independent Schrödinger equation for a ground state system is:
�̂�Ψ0 = 𝐸0Ψ0 19
where the wavefunction describing the spatial distribution of the electronic orbitals is the
eigenfunction for the Hamiltonian operator. The ground state energy is returned as the
eigenvalue of the wavefunction.
The Hamiltonian operator incorporates a number of terms representing both the
kinetic and potential energy of the system.76 In the simplest of cases, these terms include the
kinetic energy of the electrons, the kinetic energy of the nuclei, the attractive electrostatic
interaction between the electrons and nuclei, the repulsive electrostatic interaction between
Chapter 2 – Instrumentation and Methodology
31
electrons and electrons, and the repulsive electrostatic interaction between nuclei. For 𝑀
nuclei and N electrons, the Hamiltonian operator is thus given by (in atomic units)76:
�̂� = −∑∇𝑖
2
2− ∑
∇𝐴2
2𝑀𝑎+ ∑ ∑
𝑍𝐴
𝑟𝑖𝐴
𝑀
𝐴=1
𝑁
𝑖=1
𝑀
𝑖=1
+ ∑∑1
𝑟𝑖𝑗
𝑁
𝑗>𝑖
𝑁
𝑖=1
+ ∑ ∑𝑍𝐴𝑍𝐵
𝑟𝐴𝐵
𝑀
𝐵>𝐴
𝑀
𝐴=1
𝑁
𝑖=1
20
where 𝑍 is the charge on a given nucleus, and 𝑟 is the distance between two given particles.
It is possible to see that in the preceding expression, when a greater quantity of nuclei
and electrons that are present in the system, the problem becomes extremely complicated. It
is for this reason that the Schrödinger equation for relatively large systems cannot be solved.
In order to overcome this critical challenge, the Born-Oppenheimer approximation is
applied.77 Some assumptions inherent in the Born-Oppenheimer approximation are: 1. there
is a high ratio of electrons present compared to the number of nuclei; and 2. That an electron
is several orders of magnitude less massive than a nucleus. In general, this approximation
means that electrons have the ability to change their position instantaneously with respect to
the relatively slow motion of the nuclei. This assumption effectively separates the electronic
motion from the nuclear motion and considerably simplifies the Schrödinger equation by
only incorporating the electronic terms.
While the electronic Hamiltonian appears to be simpler (and, indeed, it is), the
wavefunction still cannot be solved for molecules or atoms with more than two electrons.
However, it does form the basis for employing various principles and computational methods
for solving the electronic structure as an approximation to the true solution for the ground
state of a system.
Chapter 2 – Instrumentation and Methodology
32
A key principle that must be considered while attempting to solve the Schrödinger
equation is called the variation principle.76 The variation principle states that the energy
corresponding to any trial wave function, Ψ1, will be greater than or equal to the true ground
state energy of the system. By using the variation principle, it is possible to start with a known
trial wave function, and iteratively minimize the energy such that the resulting trial wave
function resembles the true wave function as much as possible. The energy expression can
then be parameterized by a value of 𝜆, where the trial energy is calculated for each value of
𝜆. The lowest energy obtained is assumed to be closest to the true energy, satisfying the
convergence requirement.
Hartree-Fock (HF) theory was introduced as a means of solving the Schrödinger
equation using simplified wavefunctions to estimate the true energy eigenvalue of any
system with 𝑁 number of electrons. HF theory is a computationally feasible system because
rather than each electron feeling the Coulombic repulsion of every other electron
individually, it essentially considers only the average repulsion felt by a single electron over
the total field of all of the other electrons in the molecule.
It is possible to separate the Hamiltonian in terms of a product of all of the individual
electrons. In order to do this while satisfying the necessary antisymmetric property of the
wave function, a Slater determinant is used. Spin orbitals are introduced when the spin of
each atom is considered. The spin orbital depends on both spatial coordinates as well as the
spin quantum number, 𝑚𝑠. The spin orbitals are all represented by the four coordinate vector
𝐱. As previously mentioned, a spin can have two states, 𝛼 or 𝛽. The spin orbital is represented
by 𝜒𝑖(𝐱𝑖), for each electron, 𝑖. The antisymmetry of the wavefunction can be satisfied if the
wavefunction is expressed in terms of a Slater determinant78, where the spin orbitals and the
Chapter 2 – Instrumentation and Methodology
33
electronic coordinates are represented in the columns and rows, respectively. The Slater
determinant provides a wavefunction that is antisymmetric, meaning the electrons cannot
occupy the same state. Eqn. 21 shows the Slater determinant representing the Hartree-Fock
wavefunction.
Ψ(𝐱1, 𝐱2, … , 𝐱𝑁) =1
√𝑁![
𝜒1(𝐱1) 𝜒2(𝐱1) ⋯ 𝜒𝑁(𝐱1)𝜒1(𝐱2) 𝜒2(𝐱2) ⋯ 𝜒𝑁(𝐱2)
⋮ ⋮ ⋱ ⋮𝜒1(𝐱𝑁) 𝜒2(𝐱𝑁) ⋯ 𝜒𝑁(𝐱𝑁)
] 21
The HF energy can now be solved in terms of the molecular orbitals in the Slater
determinant. The wavefunction represented by the Slater determinant which has the lowest
possible energy, according to the variation principle, is the wavefunction that most closely
resembles the true wavefunction. In order to obtain the lowest energy Slater orbital, the
variation principle must also be applied to minimize the spin orbitals. However, in order to
solve this energy expression, something must be known about the spin orbitals beforehand,
which is not the case. As such, an initial guess is made, and the spin orbital energies are then
iteratively minimized through basis sets.
Basis sets are sets of functions which are used to build the HF wave function. The
HF wave function is expressed as a Slater determinant formed from each individual
molecular orbital. Roothaan expressed the spin orbital in terms of a basis set.79
A contracted Gaussian function is essentially designed to reproduce a Slater
functional while minimizing computational costs. 76 Thus, a Slater S-type orbital, using the
aforementioned parameters to mimic real Slater functionals, with 𝑀 Gaussian functions, is
referred to an STO-MG basis set. An increased size of the contracted Gaussian results in a
Chapter 2 – Instrumentation and Methodology
34
better fit with a Slater functional. However, the increase comes at a severe computational
cost, and represents mainly the core orbitals which are generally not of relevance.
Consider the basis set, 6-311++G(d,p). This basis set is composed of 6 Gaussian
functions in each of the core orbitals, 3 tight functions, 1 intermediate function and 1 diffuse
function. The latter three functions are used to replicate the decay of the Slater-type basis
sets. In this particular case, additional diffuse functions are added to each heavy atom (+),
and diffuse functions are added to hydrogen (++). Finally, there is a set of d-type polarization
functions added to the heavy atoms (before the comma) and p-type polarization functions
added to the hydrogens (after the comma). The 6-311++G(d,p) basis set includes polarization
functions, diffuse functions and it is triple-zeta, so it is used in this work to provide
calculations for cluster model analysis. Other basis sets are possible, such as Dunning’s more
modern correlation consistent basis sets80, but these come at a higher computational expense.
These basis sets are named by their zeta-level, cc-pVXZ, where X is D (double-zeta), T
(triple-zeta), etc. The term “aug” may be added to add diffuse functions in a similar way to
the ++ notation.
Each spin orbital has an eigenvalue obtained using the Fock operator, 𝐟(𝐱𝑖). The
operator acts on the spin orbital wavefunction forming the Hartree-Fock equation,
𝐟(𝐱𝑖)𝜒𝑖(𝐱𝑖) = 휀𝑖𝜒𝑖(𝐱𝑖) 22
where the Fock operator is given by
Chapter 2 – Instrumentation and Methodology
35
𝑓(𝐱𝑖) = −∇𝑖
2
2− ∑
𝑍𝐴
𝑟𝑖𝐴
𝑀
𝐴=1
+ ∑[𝐽𝑏(𝐱𝑖) − 𝐾𝑏(𝐱𝑖)]
𝑁
𝑏=1
23
The sum of all of the spin orbital energies will therefore give an expression
representing the sum of all of the single electron kinetic energies, as well as the sum of all
the double electron Coulomb and exchange energies, from the 𝐽𝑏 and 𝐾𝑏 terms, respectively.
Thus, the HF energy for the system can be expressed as
𝐸𝐻𝐹 = −∇𝑖
2
2− ∑
𝑍𝐴
𝑟𝑖𝐴
𝑀
𝐴=1
+1
2∑∑[𝐽𝑏(𝐱𝑖) − 𝐾𝑏(𝐱𝑖)]
𝑁
𝑗=1
𝑁
𝑖=1
24
2.2.2 Møller-Plesset Perturbation Theory
Due to the single-Slater restriction of HF theory, the Hamiltonian does not give the
full description of the wavefunction representing the system in question. Møller-Plesset (MP)
perturbation theory81,82,83,84,85 is a post-HF method which introduces a significant amount of
improvement over HF by incorporating electron-correlation to the solution of the
wavefunction. It is a form of perturbation theory, meaning that it adds the correction to the
reference wavefunction by expressing the perturbation as the difference between the desired
true Hamiltonian and the reference Hamiltonian, which is the sum of the Fock operators
obtained by HF theory. The general case, the desired Hamiltonian is represented as the
original unperturbed HF Hamiltonian, 𝐻0, affected by a perturbation, 𝑉:
Chapter 2 – Instrumentation and Methodology
36
𝐻 = 𝐻0 + 𝜆𝑉 25
where 𝜆 is an ordering parameter.
The value of the perturbation is given by76:
𝑉 = ∑∑1
𝑟𝑖𝑗− ∑{∑[𝐽𝑏(xi) − 𝐾𝑏(x𝑖)]
𝑁
𝑏=1
}
𝑁
𝑖=1
𝑁
𝑗>𝑖
𝑁
𝑖=1
26
MP methods are usually named after the order by which the calculation is performed,
with MP2 and MP3 being calculations of second and third order correction to the energy.
Even higher order corrections can often be obtained, but are not commonly used due to the
costly nature of these calculations. MP1, representing first order perturbation theory, simply
regenerates the HF wavefunction, and consequently is not used.
MP2, the second-order correction to the wavefunction, is commonly used MP method
due to its relatively high degree of accuracy in representing the true Hamiltonian, at a
relatively low cost. The cost is reduced because this method uses the information obtained
during an HF calculation in the new calculation. Increasing the perturbation order to the
infinite degree, using an infinite basis set, will theoretically yield a perfect wavefunction
describing the molecular system in question.
2.2.3 Density Functional Theory
Density functional theory (DFT) is able to provide the ground state properties of most
systems and is one of the best methods for computing these properties. Instead of calculating
Chapter 2 – Instrumentation and Methodology
37
the energy using the orbital wavefunctions in the Schrödinger equation, DFT depends on the
electronic density of a system to determine its total energy. This approach was first proposed
by Hohenberg and Kohn86 later to be developed into the DFT method. 87 It has since become
one of the most popular, if not the leading method, for solving complex computational
problems involving large chemical systems.
As stated, DFT uses the electron density to solve the energy of the system, and not
the wavefunction. This was developed to avoid solving the orbital wavefunctions for every
electron, as is the case in HF theory. Since the electron density simply depends on three
dimensional coordinates, unlike HF theory, where each orbital has three spacial coordinates
as well as a spin coordinate, the computational challenge become much less cumbersome.
It was shown that the density functional could be used to solve the electronic energy
of a system. 86,87 The density function 𝜌(𝑟 ) is put into an energy functional, so as to obtain
an energy.
𝐸𝐷𝐹𝑇 = 𝐸[𝜌(𝑟 )] 27
In DFT, the density functional is not known, but various functionals are developed
and tested to give the best possible answers for various scenarios. The general form of the
functional is given as76:
𝐸[𝜌] = 𝑇𝑠[𝜌] + 𝐸𝑁𝑒[𝜌] + 𝐽[𝜌] + 𝐸𝑋𝐶[𝜌] 28
In the preceding expression, the energy functional depends on the terms incorporating
the kinetic energy, 𝑇𝑠[𝜌], the electron-nucleus attraction potential, 𝐸𝑁𝑒, the Coulombic
Chapter 2 – Instrumentation and Methodology
38
interaction between electrons, 𝐽, and the exchange-correlation, 𝐸𝑋𝐶. All of these functionals
are simply added together to obtain the total DFT energy.
In order to ensure the antisymmetry principle is obeyed, spin is introduced. 87 This is
found in the 𝑇𝑠 functional, where the electrons are assumed to be non-interacting. The
electronic density is obtained through this approach, but introduces some approximation to
DFT due to its reliance on HF theory.
The functional representing nuclear attraction is simply the interaction between the
nucleus and the electron density over all space. The Coulombic repulsion term is similar in
that it is the repulsion between two given electron charge distributions over a given area.
Finally, the exchange correlation term, 𝐸𝑋𝐶, accounts for the correction to the energy
due to the exchange energy (which is already treated in HF but not directly in DFT) as well
as the fact that there is indeed electron correlation that is not incorporated into the kinetic
energy term. The exchange-correlation functional is not known; it can, however, can be
guessed.
There are many different types of DFT, each one differing in its approach to the
exchange-correlation correction. The simplest is known as the Local Density Approximation
(LDA).76 In this approach, the charge felt by the electron density is assumed to be constant
over the space at which each point in the electronic density is probed, an unrealistic prospect.
An improvement over LDA, known as the Generalized Gradient Approximation88
(GGA) is used in this work. In this case, the exchange-correlation functional is dependent
on both the electron density and the derivative thereof, which gives the change of the electron
Chapter 2 – Instrumentation and Methodology
39
density over space. This class of functionals gives a better picture of the electron density over
space as it better reproduces the true state of the system.
The best attempt at approximating the exchange-correlation functions is through the
hybrid DFT approach. In short, hybrid DFT utilizes a bit of everything, so to speak. In fact,
this class of functionals incorporates both exchange from HF theory as well as correlation
from DFT, and other sources depending on the functional. One of the most popular
functionals is B3LYP.89,90 In this functional, the HF exact exchange is used, as well as the
LDA exchange and correlation. The GGA term is simply the LYP correlation functional. The
generalized expression is given as:
𝐸𝑋𝐶𝐵3 = (1 − 𝑎)𝐸𝑋
𝐿𝑆𝐷𝐴 + 𝑎𝐸𝑋𝐻𝐹 + 𝑏∆𝐸𝑋
𝐵88 + (1 − 𝑐)𝐸𝐶𝐿𝑆𝐷𝐴 + 𝑐∆𝐸𝑐
𝐺𝐺𝐴 29
where 𝑎, 𝑏, and 𝑐 are variable parameters.
DFT has difficulty modelling certain interactions. In general, DFT has difficulty
modelling long range interactions. 91 For example, radical-molecule interactions are prone to
error due to limited exchange modelling the charge transfer. 92 Similar issues arise with other
noncovalent interactions because DFT cannot properly model electron density over longer
distances, and so the exchange potential is represented by −0.2
𝑟, where the ideal case would
be seeing the exchange potential treated as −1
𝑟. 91,91 However, some hybrid DFT functionals
attempt to overcome these problems. These include BHandHLYP93, which uses a mixture of
both DFT and HF exchange energies and CAM-B3LYP94 (CAM = Couloumb attenuating
method), which introduces long range corrections in order to better treat noncovalent
interactions. PBE is a functional which has both exchange and correlation correction
Chapter 2 – Instrumentation and Methodology
40
incorporated. When this functional is corrected for long range, it is referred to as PBE, or
LC-PBE95,96,97 ( = 0.40 a.u.), depending on the corrections used. The M0598 and M0699
family of functionals are meta-GGA approaches to the exchange and correlation correction.
The preceding functionals have all been used in this thesis to evaluate the interaction
energies, as well as the NMR parameters of various simple compounds.
2.2.4 Computation of NMR Parameters using DFT
DFT is a useful computational method for calculating the magnetic properties of
atoms and molecules when they are under the influence of a magnetic field. In computing
properties such as magnetic shielding and spin-spin coupling, the chemist has the ability to
predict the outcome of NMR experiments. Additionally, DFT computational results may
provide complementary information to support the experimental findings of an NMR study.
When a molecule is subjected to an external magnetic field, the electrons are
perturbed in such a way that their properties are altered by the field. In DFT, the magnetic
properties of the electrons can be derived from the first and then second derivatives of the
total energy of the system with respect to two different perturbations, under the assumption
of a static magnetic field. In other words, all of the information needed to obtain magnetic
properties are within the wavefunction of the system.100
Nuclear shielding constants as well as indirect spin-spin coupling constants are
obtained from the derivative of the electronic energy of the system with respect to the
magnetic induction, and the nuclear magnetic moments to obtain the various contributions
to the J-coupling. 101 The second derivative is performed to determine further the magnetic
Chapter 2 – Instrumentation and Methodology
41
properties of the system. This is essentially derived from the electronic Hamiltonian for the
system, whereby the Hamiltonian is altered slightly for the dependence on the external
magnetic field.
DFT is, of course, an approximation method to solve the total energy of the system.
In doing so, it uses basis sets in order to represent molecular orbitals. When an infinite size
basis set is used, a perfect solution can be obtained. However, this is not possible, and
introduces the so-called “gauge origin problem” to the calculation of NMR parameters. It is
a problem that exists as a result of improper description of the magnetic field.102 This is
solved through the implementation of the gauge-invariant atomic orbitals (GIAO) method103,
being the default option in the Gaussian software.
2.2.5 Gauge Including Projector Augmented Wave DFT Calculations
Gauge Including Projector Augments Waves (GIPAW) DFT calculations 104 are
conducted on known crystal structures to obtain NMR parameters. GIPAW DFT is important
because it is able to account for the long-range effects of the crystal lattice on the NMR
properties, giving rise to more accurate results than in methods using single molecules.
GIPAW DFT is implemented in the CASTEP-NMR software code.105
Periodic boundary conditions are used to compute the total energy of a bulk
crystalline system. Since a crystalline material is made up of repeating unit cells, GIPAW
DFT is extremely useful for calculating NMR parameters of crystal structures in the solid
state. The main advantage of GIPAW DFT is that it is able to produce fairly accurate results
Chapter 2 – Instrumentation and Methodology
42
at a reasonable computational cost, whereas other traditional methods of DFT would not be
able to achieve similar results without astonishing computational cost.
In the GIPAW method, there are several factors that must be considered. First, a plane
wave basis set must be specified. Plane wave basis sets are used because of their improved
treatment of periodic systems. In addition, in order to minimize the number of nodes in the
core wavefunction due to the higher kinetic energy of the electrons, pseudopotentials provide
an alternative that replicates the core such that the computation can proceed better.106 Finally,
a cut-off energy is set in order to define the level of convergence for the calculation.
2.2.6 Counterpoise Correction
Counterpoise (CP) correction107 is used in computational chemistry in order to reduce
basis set superposition error (BSSE). When calculating bimolecular interactions, it is
important to consider the effect of BSSE because in the calculation of the complex, there
will be an artificial lowering of the overall energy because of the sharing of basis functions
between the nearby monomers.108 CP-correction provides a good way to correct for this error,
showing good results for noncovalent interactions at higher level calculations, such as
MP2.109
In the CP-correction program, the energy is calculated a number of times in Gaussian:
1. Dimer
2. Monomer 1 with dimer centred basis set (DCBS 1),
3. Monomer 2 with dimer centred basis set (DCBS 2)
Chapter 2 – Instrumentation and Methodology
43
4. Monomer 1 with monomer centred basis set (MCBS 1)
5. Monomer 2 with monomer centred basis set (MCBS 2)
The CP-corrected energy is thus given by a simple formulation of all of the calculated
energies110 (eqn. 30).
𝐸𝐶𝑃 = 𝐸𝑑𝑖𝑚𝑒𝑟 − 𝐸𝐷𝐶𝐵𝑆1 − 𝐸𝐷𝐶𝐵𝑆
2 30
The resulting energy value obtained from a calculation is the interaction energy (as a
function of intermolecular distances or angles). This is, however, different from binding
energy. In order to find the binding energy, the monomers are geometry optimized, then the
dimer is again geometry optimized at a fixed distance (2.825 A). The resulting energy is the
binding energy. The interaction energy is then the energy obtained when the geometries are
then frozen and the interaction distance is changed.
The NMR values are obtained from the output files from the dimer calculation. There
has been a study looking into the impact of BSSE on magnetic shielding constants. However,
for 13C and 15N, these corrections are normally on the order of 0.2 ppm for magnetic shielding
and 0.01 Hz for J-coupling (own data). As such, for the purpose of revealing NMR trends,
the CP-correction is not used to obtain corrected NMR parameters; only interaction energies.
2.3 Experimental Methodology of SSNMR
2.3.1 Experimental Setup
The NMR spectrometer (Figure 9) consists of several components which, when
acting together, allow the user to collect an NMR spectrum of a compound of interest,
Chapter 2 – Instrumentation and Methodology
44
whether it be in the liquid state or in the solid state. The major components of interest are the
magnet, the transmitter, the probe and the receiver.
The magnet provides the experiment with a strong, essentially homogenous magnetic
field in order to induce the Zeeman interaction, the fundamental process which gives rise to
the NMR transition. The energy corresponding to the NMR transition is dependent on the
strength of 𝐵0, so in the absence of a magnetic field, it would be difficult to observe an NMR
spectrum.
Figure 9. A 9.4 T NMR spectrometer magnet for the solid state. The superconducting coil is
found within the large cylindrical container, which also houses the cooling liquid.
Chapter 2 – Instrumentation and Methodology
45
2.3.2 Magic Angle Spinning
Magic angle spinning is a technique used in SSNMR which has the ability to reduce
or eliminate the anisotropies of certain NMR interactions such as dipolar coupling and
chemical shift anisotropy, which are orientationally dependent.111,112,113 MAS mimics the
isotopic tumbling of molecules in solutions through motional averaging. In solids, MAS can
reduce the anisotropies of chemical shift anisotropy, heteronuclear dipolar coupling
anisotropy and the J-coupling interaction anisotropy.111 Finally, the quadrupolar effect is
only partially averaged. In most cases, MAS has the average effect of sharpening the NMR
signals to yield liquid-like spectra. Its importance is very clear when it comes to the analysis
of complex spectra with many peaks at different chemical shifts. It is thus useful in chemical
shift assignment, or when changes in chemical shifts must be probed. However, due to the
reduction of the anisotropies, MAS has the effect of reducing the ease of observing some
anisotropic NMR parameters. Therefore, often times the NMR spectroscopist will also
perform static NMR experiments, where the sample remains motionless in the coil.
The need for MAS comes from the dependence of the angle of the PAS of certain
NMR interactions, such as magnetic shielding, with respect to 𝐵0 (eqn. 31). This dependence
is contained within a term in each of the respective Hamiltonian operators.
3 cos2 𝜃 − 1 31
𝜃 is the angle between the magnetic field and the z-axis of the interaction tensor.
Consequently, when 𝜃 = 54.74o, or the Magic Angle, the term is forced to zero. Thus, when
a sample is rotated around the magic angle axis, the averaging of the anisotropies occurs.
Chapter 2 – Instrumentation and Methodology
46
In order for the procedure to work, the spinning rate must be fast compared to the
anisotropy of the interaction, because there is a dependence of the cos 𝜃 term on the angular
velocity of the spinning rotor.114,115 As such, the faster the spinning speed, the more isotropic
the spectrum becomes. 59 A set of spinning side bands will be present, separated from the
isotropic peak by intervals of the spinning speed, in Hz. At the time of writing this thesis,
some of the fastest spinning rates of 111 kHz and 110 kHz that have been made commercially
available have been achieved by Bruker and JEOL, on their 0.7 mm116 and 0.75 mm117
CP/MAS probes, respectively.
2.3.3 Sensitivity Enhancement
2.3.3.1 Cross-Polarization
Cross-polarization (CP) is a technique used to improve the signals of spin-1
2 nuclei
which often have low natural abundance (n.a.) or are sparse within the sample (such as in the
case of 13C, n.a.= 1.1%) This technique is made possible due to the possibility for some
nuclei to transfer their polarization to other nuclei. In cases where the n.a. of the NMR active
nucleus is very low (< 1%), a CP experiment can drastically increase the signal-to-noise
ratio, and decrease the experimental time required in order to obtain decent results.
A CP experiment takes advantage of the fact hydrogen atoms possess an inherently
larger magnitude of polarization compared to other atoms of interest, such as 13C, 15N, and
31P, among others. This abundance in polarization is due to the protons’ gyromagnetic ratio,
, which is much larger than most other NMR active nuclei. The CP experiment will work
when the pulse applied to both the proton frequency channel and the frequency channel of
Chapter 2 – Instrumentation and Methodology
47
the nucleus of interest satisfies the Hartmann-Hahn matching condition118, meaning, the
nuclear precession frequencies become matched, thereby allowing a transfer of spin
polarization.
The Hartmann-Hahn matching condition can be demonstrated by first recalling that
E depends on the gyromagnetic ratio and the magnetic field. If two nuclear spins, 1H and
R, are coupled, and the application of an RF field induces local magnetic fields, then
ℎ𝑣 H1 = 𝛾 H1 𝛽1( H1 ) 32
ℎ𝑣𝑅 = 𝛾𝑅𝛽1(𝑅) 33
where 𝐵1 is the oscillating field generated by the respective nuclei. The Hartmann-Hahn
condition is fulfilled when:
𝛾 H1 𝐵1( H)1 = 𝛾𝐵𝐵1(𝑅) 34
so these two terms are matched by a common rf pulse.
A typical single pulse program using CP is shown in Figure 10. Following the 90o
pulse, a contact pulse is applied during which there is a transfer of polarization from the spin
A to spin B. Proton decoupling is applied during acquisition to ensure that maximum
sensitivity is gained on the nucleus of interest without interference from proton coupling.
Chapter 2 – Instrumentation and Methodology
48
Figure 10: Typical single pulse cross polarization pulse program. A 𝜋
2 pulse is applied to the
proton channel, followed by a 1H 13C contact time. This is followed by the acquisition
period coinciding with decoupling from the protons.
2.3.3.2 Data Acquisition Periods
A physical parameter that can be changed is the number of transients, or scans, that
are obtained in the experiment. The signal to noise ratio is very much dependent on this
number. As the number of transients increases, so does the signal-to-noise ratio.
Consequently, depending on the natural abundance of the nuclide being observed, it is typical
for an experiment to acquire hundreds, if not thousands of samplings to obtain a good end
signal. The signal intensity can be described as increasing as the square root of the number
of scans (eqn. 35).
𝑆
𝑁= √𝑛scans 35
Therefore, four times the number of scans is required to double the signal intensity
with respect to the background noise. However, the preceding expression shows that the
Chapter 2 – Instrumentation and Methodology
49
signal to noise ratio becomes limited as a function of time. As such, it is necessary to balance
the experimental time with the desired signal intensity.
Figure 11. The increase of the signal-to-noise ratio as a function of the number of time
dependent scans. Initially, the signal intensity grows rapidly, but as time continues to
increase, the interval at which the signal gain is achieved becomes impractically long.
2.4 Experimental Methods
2.4.1 Sample Preparation
Crystal structures exhibiting carbon tetrel bonds were selected from the CSD.
Conquest version 1.17 was used in conjunction with CSD version 5.36 with the November
2014 update, and the structures were visualized in Mercury version 3.5.1. The compounds
were chosen based on the criteria described in Chapter 3.
Salts containing tetrel bonds were investigated: sarcosinium tartrate, sarcosine
maleate and of N,N,N’,N’-tetramethylethylenediammonium succinate succinic acid.
0
20
40
60
80
100
120
140
160
180
200
0 10000 20000 30000 40000
Sig
na
l-to
-no
ise
Ra
tio
Number of Transients
Chapter 2 – Instrumentation and Methodology
50
Sarcosine was obtained from Sigma-Aldrich and used without further purification, and the
salts were collected according to the published procedures.44, 119,120
2.4.2 Powder X-ray Diffraction – Experimental Methods
The sample purity was confirmed by powder X-ray diffraction, using a Rigaku
Ultima IV X-ray diffractometer, with the Bragg-Brentano method with a monochromator
with CuK1 radiation ( = 1.54060 Å). Diffractograms were collected at room temperature
(298 ± 1 K) and with 2 values ranging from 2° to 5°, to 80° in increments of 0.02°.
Diffractograms were analyzed using the Rigaku PDXL 2 software and compared to existing
diffractograms in the PDF-2 2.1302 database and simulations generated using the Mercury
version 3.5.1 software provided from the Cambridge Crystallographic Data Centre (CCDC)
(CCDC entry numbers are 660888 and 159986, 142944 and 237950 for sarcosine,
sarcosinium tartrate, N,N,N’,N’-tetramethylethylenediammonium dichloride and of
N,N,N’,N’-tetramethylethylenediammonium succinate succinic acid, respectively).
2.4.3 Cluster Model Analysis
Computations on a library of model compounds were done several times, for
comparison, using B3LYP, MP2, BH&HLYP, CAM-B3LYP, LC-PBE, and LC-PBE-D3
(D3 refers to the addition of Grimme’s dispersion121) methods with the Gaussian 09
software122 on the Wooki cluster at the University of Ottawa. While the MP2 method cannot
calculate the NMR parameters, it is chosen as a method for comparing the energy calculated
by various DFT methods because it is able to properly treat noncovalent interactions.
Chapter 2 – Instrumentation and Methodology
51
In addition, a series of other functionals were also used to establish a cost benchmark
to identify the best functionals for calculating tetrel bonding energies (Table 2). The model
compounds were constructed and visualized via GaussView 4.1 software for Microsoft
Windows.123 All calculations were conducted with the 6-311++G(d,p) basis set. The tetrel
bond donor and acceptor moieties were each first geometry optimized using both density
functional theory (DFT) methods, or MP2. The DFT optimized precursors were combined
to form the tetrel-bonded systems that would be examined by various DFT methods, and the
MP2 optimized precursors were combined into models that would be analyzed via MP2. In
all cases the carbon tetrel bond length was set to 2.825 for geometry optimization. These
tetrel bonded models were then again geometry optimized by both DFT and MP2 methods
using counterpoise (CP) correction. Once optimized, the DFT and MP2 NMR parameters
were calculated. The GIAO method was used for magnetic shielding, specifying iop33(10=1)
in order to compute paramagnetic and diamagnetic contributions to the magnetic shielding
constants. Examples of Gaussian input files are in Appendix II – Sample of Computation
Input Files. EFGShield version 4.2 was used to extract the NMR parameters.124 Magnetic
shielding constants were then converted to chemical shift values with respect to the shielding
constant for tetramethylsilane (TMS), 184.1 ppm.125 Total J-coupling values were extracted
manually from the Gaussian output files calculated by DFT methods when the “spinspin”
keyword was specified. Taking into account basis set superposition error (BSSE), CP-
corrected interaction energies were obtained in units of kcal/mol and reported in this work.
Chapter 2 – Instrumentation and Methodology
52
2.4.4 Solid-State NMR
13C solid-state NMR was conducted at 9.4 T (𝜈𝐿(13C) = 100.613 MHz) under MAS
conditions (°) on an AVANCE III NMR spectrometer. Cross polarization
experiments (𝜈𝐿(1H) = 400.130 MHz) were performed with a spinning rate of 6 kHz in a
Bruker 4 mm HXY probe. Spectra were referenced externally to glycine at 176.4 ppm. In
each case, the contact time was 5000 s and the proton 90-degree pulse was 3.00 s. Several
thousand transients were typically acquired using a relaxation delay of 5 s.
Figure 12. A 4 mm MAS rotor compared to a Canadian Penny for scale. The cap of the rotor
is winged so that it may spin using a high pressure air stream. The spinning speed is adjusted
using an MAS controller fit onto the spectrometer console.
2.4.5 GIPAW DFT
GIPAW DFT calculations were carried out using the CASTEP-NMR software version
4.4126,105 on the Wooki cluster at the University of Ottawa. This was done in order to properly
treat the effects of the crystal lattice. Crystallographic information files were imported into
Materials Studio v. 4.4 (Accelrys) to generate input files. In all cases, the generalized gradient
approximation (GGA) with the functional of Perdew, Burke, and Ernzerhof (PBE)127 using
on-the-fly ultrasoft pseudopotentials128,129 was employed. Geometry optimization for the
hydrogen atoms, followed by NMR calculations on the sarcosine salts, were performed with
Chapter 2 – Instrumentation and Methodology
53
a 550.0 eV cutoff at the “fine” setting for the k-point grids. The calculation for sarcosine was
conducted using a 610.0 eV cutoff at the “ultra-fine” setting for the k-point grids. No
geometry optimization was performed for sarcosine. NMR parameters were extracted from
the CASTEP NMR output file using EFGShield version 4.2.124
Chapter 3 – Results and Discussion
54
Chapter 3 - Results and Discussion
3.1 Computational Investigations of NMR Trends in Tetrel Bonds
In this study, computational investigations were performed on a library of model
systems containing carbon tetrel bonds (Figure 14). It was previously demonstrated that
regions of negative charge energetically favour a weak interaction with the methyl carbon of
interest, especially when the methyl carbon is bonded to a strong electron-withdrawing
substituent.54 As discussed by Torres and DiLabio, DFT methods such as B3LYP often
cannot accurately describe medium to long range non-covalent interactions without some
sort of correction.91 Yet, the use of DFT is highly desirable because it can provide rapid and
accurate J-coupling values, an important NMR parameter providing structural information,
which can be used to probe the tetrel bond. A number of solutions have been offered to
overcome the shortfalls of DFT, including the use of dispersion correction,121 and the
packaging of improved exchange-correlation, as in the case of the M06 suite of functionals.91
In order to describe the tetrel bonding interaction energy, a study was performed to determine
a set of density functionals that could best represent the tetrel bond.
Model 6 (Figure 14) was chosen as the standard for this test. It was chosen due to its
relatively simple structure, and because it possesses a negative charge. The carbon tetrel bond
length was fixed at 2.825 Å, and the geometry was optimized by B3LYP/6-311++G(d,p)
with CP correction. The CP corrected bonding energy was obtained, using the 6-
311++G(d,p) basis set, for each of the functionals that were tested (Table 2). In each case,
the bonding energy was compared to the QCISD bonding energy, -2.72 kcal/mol.
Chapter 3 – Results and Discussion
55
Table 2. Functionals compared to QCISD in order to set a benchmark for determining the
highest performing functional as it applies to carbon tetrel bonding.
Density Functional
Correction
CP
corrected
energy
/ a.u.
CP
corrected
bonding
energy
/ kcal/mol
M06-2X D3 -285.03 -4.53
M06-2X - -285.03 -4.40
M06-HF130,131 - -285.05 -4.61
LC-ωPBE D3 -284.92 -4.74
LC-ωPBE - -284.98 -2.57
CAM-B3LYP D3 -284.98 -5.21
CAM-B3LYP - -285.05 -3.33
BHandHLYP - -284.99 -3.04
B3LYP D3 -285.10 -4.77
B3LYP - -285.17 -2.45
HF - -283.51 -1.83
CCSD132,133 - -284.42 -2.72
QCISD134 - -284.43 -2.72
A few functionals provide results within a relatively small difference of 0.5 kcal/mol
from the bonding energy obtained using QCISD (-2.72 kcal/mol), these being LC-PBE,
B3LYP, and BHandHLYP. CAM-B3LYP is also close but yielded an energy difference of
0.61 kcal/mol. Given the relative costs (Figure 13), the functionals that were chosen to
proceed representing a good mix of correlation and dispersion corrections that were chosen
for further calculations were B3LYP, BHandHLYP, CAM-B3LYP, LC-PBE and LC-
PBE-D3. We note that all of the M06 functionals took significantly longer and yielded
results which were further away in magnitude from the QCISD result.
Chapter 3 – Results and Discussion
56
Figure 13. Cost analysis of the various methods used in the test study on model 6. The red
hashed line represents the energy difference cut-off for this study at 0.5 kcal/mol, as
compared to the energy obtained in the QCISD calculation. All energies are at a tetrel bond
distance of 2.825 Å. The time taken for the QCISD calculation was 5,232 s.
Chapter 3 – Results and Discussion
57
Figure 14. Model compounds containing carbon tetrel bonds between methyl carbons and
oxygen-containing functional groups.
To explore trends in the NMR parameters, the LC-PBE, LC-ωPBE-D3,
BHandHLYP, B3LYP functionals, as well as the MP2 method, were used to perform
Chapter 3 – Results and Discussion
58
calculations of magnetic shielding tensors, on each of the compounds in the library (Figure
14), using the 6-311++G(d,p) basis set in Gaussian 09.122 Model structures were constructed
with carbon tetrel bond lengths increasing in 0.10 Å increments from 2.825 Å to 3.325 Å
(Figure 15), just over the sum of the vdW radii between carbon and oxygen, and carbon and
nitrogen, 3.22 Å and 3.25 Å, respectively.
Figure 15. A schematic showing how the tetrel bond lengths of the model compounds are
modified for the computations. The bond lengths are changed in 0.10 Å increments from
2.825 Å to 3.325 Å. The atomic coordinates are modified in the GaussView software.
The results for iso are presented graphically in Figure 16. At the time of this work,
in the vast majority of reported crystal structures, carbon tetrel bonds between methylamine
and oxygen have interaction lengths greater than 2.8 Å. However, there are a few cases where
the distance is shorter. The smallest value in the database is 2.591 Å,135 and the shortest
carbon tetrel bond between methylamine and a carboxylic acid is 2.825 Å.136
This analysis was done in order to expand the overall understanding of how the 13C
chemical shift of methyl group involved in a R-C···Y tetrel bond (R = C, F, N, N+1, S or S+1;
Y = O, O-1, or N) changes as a function of the interaction distance. The response of the
chemical shift to the tetrel bond angle was also assessed. The structures were constructed
Chapter 3 – Results and Discussion
59
with tetrel bond lengths of 2.925 Å, then varying the R-C···Y angle in increments of 5°
between 140° and 180°. This provides an adequate range over which to test chemical shift
response to the changing geometry of the tetrel bond and has been used previously as the
relevant range over which to search the CSD for existing tetrel bonded compounds.58
Chapter 3 – Results and Discussion
60
Figure 16. NMR computational investigations of model compounds. Calculated isotropic
chemical shifts of model compounds using (a) MP2, (b) B3LYP, (c) LC-PBE, (d) LC-
PBE-D3, (e) BHandHLYP, and (f) CAM-B3LYP are plotted against the reduced distance
parameter (rC∙∙∙Y) (top axis) and the interaction distance (d (C∙∙∙Y)) (bottom axis). Each plot
is fit by a quadratic polynomial function with R2 > 0.99 for all methods except CAM-B3LYP
(Table 12-Table 17). For spacing, data values for structures 8, 9, 13 and 14 are found in
Table 6 to Table 8 in Appendix I – Supplementary Data.
The model compounds are varied by the nature of their chemical structures and their
substituents, while the change in the C…Y tetrel bond distance remained consistent across all
of the examples (Figure 14). We also propose the use of the normalized distance parameter,
Chapter 3 – Results and Discussion
61
RX···Y, to measure the chemical shift response as well as the interaction energy as a function
of the interaction length (where the interaction distance is divided over the sum of the vdW
radii), as has been done for halogen bonds (eqn. 36).
𝑅X···Y =𝑑X···Y
∑𝑑VDW 36
Interestingly, in each case, the calculated 13C chemical shift increases quadratically
as the carbon tetrel bond length decreases, indicating of a correlation between the tetrel bond
strength and the chemical shift. This trend is not unexpected; it is reproduced experimentally
in 81Br halogen bonding, where the 81Br chemical shift increases significantly with the
shortening of the halogen bond distance, albeit with the possible competing effects of
hydrogen bonding.137 The polynomial function is stable beyond the vdW distance. The
computational data therefore suggest that, experimentally, the introduction of a carbon tetrel
bond should result in a positive 13C chemical shift on the order of up to 5 ppm. We note that
in the case of fluoro-substituted compounds (8 and 9), the computed chemical shift difference
is on the order of less than 1 ppm, albeit following the same trend. We note that while each
functional provides a different magnitude of chemical shift, they all show similar trends.
CP corrected interaction energies are reported in Figure 17. These computations
show that there is indeed a dependence of the interaction energy on the interaction distance.
Sometimes a local minimum is reached over the relevant range of distances, while sometimes
these minima reside closer or farther. However, there is no clear correlation with chemical
shift trends. Therefore, it can be expected that the presence of a tetrel bond, whether it is a
Chapter 3 – Results and Discussion
62
favourable or unfavourable interaction energetically, will provide the same chemical shift
trends as a function of distance.
A further analysis of the computed results (Figure 16) reveals that for the neutral
models (Figure 14), the chemical shift trend is largely dominated by changes in the
paramagnetic contribution, p, to the magnetic shielding constant, (Table 3). Conversely,
for the charged models, the changes in the diamagnetic contribution, d, are on the same
order of magnitude as the changes in the paramagnetic contribution. Also notable is that the
overall change in the magnitude of between B3LYP and LC-PBE is largely a result of
the change in the magnitude of the p values, reflecting the latter’s ability to better handle
longer range corrections. The paramagnetic contribution involves the mixing of virtual
orbitals with the ground electronic state (eqn. 37), while the diamagnetic contribution reflects
the structure of the ground electronic state (eqn. 38). A favourable overlapping of the ground
state orbitals (0) with the excited state orbitals (𝑛) results in paramagnetic deshielding. Given
that the overall changes to the chemical shift are very small relative to the total range of
known 13C chemical shifts, it is unproductive to attempt to further attribute the contributions
to specifics of the electronic structure of the tetrel bond.
𝜎𝑝𝛼𝛽
= −(𝜇0
4𝜋)(
𝑒2
2𝑚) ∑ {
⟨0|∑ 𝑟𝑘−3𝑙𝑘𝛼𝑘 |𝑛⟩⟨𝑛| ∑ 𝑙𝑘𝛽𝑘 |0⟩ + ⟨0|∑ 𝑙𝑘𝛽𝑘 |𝑛⟩⟨𝑛| ∑ 𝑟𝑘
−3𝑙𝑘𝛼𝑘 |0⟩
휀𝑛 − 휀01 }
𝑛≠0
37
𝜎𝑑𝛼𝛽
= (𝜇0
4𝜋)(
𝑒2
2𝑚) ⟨0|
𝑟2𝛿𝛼𝛽 − 𝑟ℎ𝛼𝑟ℎ𝛽
𝑟𝑘3 |0⟩ 38
Chapter 3 – Results and Discussion
63
where 𝜇0 is the mass of an electron, and 𝛿𝛼𝛽 is a Kroeneker delta, and the other terms are
previously defined.
Computed 13C chemical shift anisotropies (CSA, Haeberlen convention) for the
model compounds range from about 15 ppm for symmetric models (i.e., 1 and 2; (d = 3.325
Å)) to a high of almost 116 ppm for 14 (d = 2.825 Å) (Table 4). In all cases, the CSA
increases as the tetrel bond shortens.
Chapter 3 – Results and Discussion
64
Figure 17. Computed CP corrected interaction energy values vs. interaction distance of the
model compounds. Computed interaction energies using (a) MP2, (b) B3LYP, (c) LC-PBE,
(d) LC-PBE-D3, (e) BHandHLYP, and (f) CAM-B3LYP are plotted against the reduced
distance parameter (rC∙∙∙Y) (top axis) and the interaction distance (d(C∙∙∙Y)) (bottom axis). The
calculated interaction energies of the model compounds were obtained by 6-311G++(d,p)
with each respective functional. Each plot is fit by a quadratic polynomial function with R2
> 0.96 (Table 12 to Table 17 in Appendix I – Supplementary Data).
Chapter 3 – Results and Discussion
65
Table 3. Computed values of the diamagnetic and paramagnetic contributions to the
magnetic shielding constants (d, p, and t) for the model structures. Values were calculated
by B3LYP and LC-PBE using the 6-311++G(d,p) basis set.
B3LYP LC-PBE
Model
Structure
Interaction
Distance
/ Å d p t d p t
1 2.825 247.58 -79.22 168.37 247.81 -67.42 180.39
3.125 246.80 -75.34 171.47 246.71 -63.52 183.19
3.325 246.51 -73.85 172.66 246.25 -61.99 184.26
2 2.825 247.74 -79.39 168.34 246.76 -66.41 180.35
3.125 247.54 -76.10 171.44 246.59 -63.37 183.22
3.325 247.48 -74.79 172.69 246.57 -62.27 184.30
3 2.825 255.59 -110.45 145.14 257.13 -99.42 157.71
3.125 256.26 -109.89 146.37 257.69 -98.77 158.92
3.325 256.64 -109.73 146.92 258.06 -98.59 159.47
4 2.825 250.02 -103.79 146.23 251.24 -91.04 160.20
3.125 250.35 -101.54 148.81 251.20 -89.14 162.06
3.325 250.55 -100.73 149.81 251.25 -88.45 162.80
5 2.825 259.65 -114.58 145.07 262.58 -105.05 157.54
3.125 260.08 -113.92 146.16 263.34 -104.62 158.72
3.325 260.32 -113.63 146.69 263.80 -104.51 159.29
6 2.825 250.11 -104.92 145.19 251.03 -92.52 158.52
3.125 250.86 -103.60 147.26 251.76 -91.17 160.58
3.325 251.25 -103.04 148.21 252.21 -90.68 161.53
7 2.825 249.77 -112.55 137.22 250.88 -100.30 150.58
3.125 250.06 -110.15 139.91 251.02 -98.23 152.80
3.325 250.22 -109.27 140.95 251.16 -97.47 153.69
8 2.825 245.88 -198.11 47.78 248.08 -185.82 62.26
3.125 245.44 -197.46 47.98 247.18 -184.78 62.40
3.325 245.13 -197.04 48.09 246.68 -184.19 62.49
9 2.825 249.33 -182.74 66.59 249.39 -171.76 77.63
3.125 249.85 -182.97 66.88 249.83 -171.99 77.84
3.325 250.18 -183.17 67.01 250.15 -172.17 77.98
10 2.825 249.58 -113.75 135.83 251.28 -102.04 149.24
3.125 249.59 -110.56 139.04 251.06 -99.05 152.01
3.325 249.63 -109.25 140.38 251.00 -97.80 153.20
11 2.825 249.97 -86.20 163.77 250.47 -71.70 178.77
3.125 249.42 -82.79 166.64 249.92 -68.53 181.40
3.325 249.09 -81.24 167.84 249.52 -67.02 182.50
Chapter 3 – Results and Discussion
66
12 2.825 249.48 -92.30 157.18 251.46 -78.61 172.86
3.125 248.83 -90.89 157.94 250.67 -76.80 173.88
3.325 248.50 -90.14 158.36 250.21 -75.81 174.40
13 2.825 248.16 -143.09 105.07 249.13 -133.40 115.72
3.125 248.93 -142.52 106.41 249.76 -132.84 116.92
3.325 249.37 -142.40 106.97 250.15 -132.68 117.48
14 2.825 246.82 -141.52 105.30 247.78 -131.98 115.81
3.125 247.67 -141.32 106.35 248.49 -131.67 116.82
3.325 248.12 -141.22 106.89 248.87 -131.51 117.37
15 2.825 259.60 -122.14 137.46 261.51 -111.86 149.65
3.125 260.27 -121.50 138.77 262.05 -110.94 151.12
3.325 260.46 -121.03 139.44 262.21 -110.41 151.80
16 2.825 255.88 -118.03 137.85 257.54 -107.58 149.97
3.125 256.29 -117.11 139.18 257.81 -106.40 151.41
3.325 256.46 -116.64 139.82 257.94 -105.87 152.07
Chapter 3 – Results and Discussion
67
Table 4. Computed chemical shift anisotropy data for model compounds using stated functionals using the 6-311++g(d,p) basis set.
Model Structure
Functional
Interaction
Distance
/ Å 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16
MP2
2.825 20.51 21.96 56.39 52.81 57.86 58.37 66.15 26.53 30.15 71.51 32.76 39.40 106.49 112.12 73.95 73.19
2.925 19.52 20.89 56.16 52.09 57.59 57.47 65.39 26.66 30.64 69.80 31.05 38.50 106.38 111.23 72.92 72.12
3.025 18.67 19.96 55.92 51.44 57.31 56.64 64.71 26.76 31.07 68.32 29.59 37.69 106.23 110.42 71.99 71.18
3.125 17.95 19.16 55.68 50.88 57.03 55.90 64.12 26.85 31.43 67.05 28.35 36.97 106.05 109.68 71.16 70.35
3.225 17.36 18.49 55.46 50.39 56.76 55.23 63.61 26.91 31.75 65.97 27.30 36.35 105.86 109.04 70.44 69.64
3.325 16.87 17.93 55.25 49.98 56.51 54.65 63.18 26.97 32.01 65.06 26.42 35.82 105.69 108.47 69.80 69.02
B3LYP
2.825 22.00 23.54 60.60 54.81 61.56 59.72 66.54 27.83 32.16 74.61 40.34 51.75 112.30 118.57 77.55 76.81
2.925 21.03 22.45 60.48 54.16 61.48 58.89 65.85 27.99 32.48 72.59 38.48 51.12 112.32 117.67 76.60 75.80
3.025 20.16 21.50 60.32 53.56 61.35 58.16 65.21 28.13 32.75 70.85 36.89 50.52 112.24 116.85 75.73 74.90
3.125 19.43 20.68 60.14 53.02 61.20 57.52 64.65 28.24 32.97 69.37 35.53 49.98 112.12 116.10 74.96 74.10
3.225 18.81 19.98 59.96 52.55 61.03 56.96 64.16 28.32 33.16 68.13 34.39 49.49 111.98 115.44 74.27 73.40
3.325 18.30 19.40 59.79 52.14 60.87 56.46 63.74 28.40 33.32 67.09 33.44 49.06 111.84 114.85 73.66 72.79
LC-PBE
2.825 18.32 19.89 56.12 50.89 57.72 56.71 61.96 31.25 34.34 67.89 31.81 43.04 109.89 115.91 73.48 72.67
2.925 17.38 18.83 55.92 50.06 57.46 55.69 61.26 31.48 34.66 66.21 30.16 42.20 109.85 115.01 72.38 71.54
3.025 16.57 17.92 55.70 49.35 57.18 54.77 60.63 31.66 34.93 64.76 28.76 41.43 109.74 114.18 71.39 70.55
3.125 15.89 17.14 55.47 48.72 56.90 53.94 60.08 31.79 35.14 63.53 27.58 40.76 109.59 113.43 70.53 69.68
3.225 15.33 16.49 55.25 48.19 56.63 53.21 59.60 31.89 35.32 62.48 26.58 40.17 109.43 112.77 69.77 68.93
3.325 14.87 15.95 55.06 47.76 56.37 52.57 59.21 31.97 35.47 61.62 25.75 39.65 109.28 112.20 69.11 68.29
LC-PBE-D3
2.825 18.32 19.89 56.12 50.89 57.72 56.71 61.96 31.25 34.34 67.89 31.81 43.04 109.89 115.91 73.48 72.67
2.925 17.38 18.83 55.92 50.06 57.46 55.69 61.26 31.48 34.66 66.21 30.16 42.20 109.85 115.01 72.38 71.54
3.025 16.57 17.92 55.70 49.35 57.18 54.77 60.63 31.66 34.93 64.76 28.76 41.43 109.74 114.18 71.39 70.55
3.125 15.89 17.14 55.47 48.72 56.90 53.94 60.08 31.79 35.14 63.53 27.58 40.76 109.59 113.43 70.53 69.68
3.225 15.33 16.49 55.25 48.19 56.63 53.21 59.60 31.89 35.32 62.48 26.58 40.17 109.43 112.77 69.77 68.93
3.325 14.87 15.95 55.06 47.76 56.37 52.57 59.21 31.97 35.47 61.62 25.75 39.65 109.28 112.20 69.11 68.29
CAM-B3LYP
2.825 21.15 22.73 59.44 53.84 60.23 58.74 65.75 28.66 32.13 73.63 37.61 47.52 112.33 118.67 77.01 76.22
2.925 20.13 21.60 59.25 53.13 60.08 57.86 65.02 28.84 32.45 71.62 35.70 46.68 112.30 117.73 75.93 75.10
3.025 19.24 20.60 59.03 52.48 59.90 57.08 64.34 28.98 32.72 69.88 34.05 45.92 112.18 116.86 74.96 74.09
3.125 18.48 19.75 58.81 51.90 59.70 56.39 63.74 29.09 32.94 68.41 32.66 45.23 112.02 116.08 74.09 73.21
3.225 17.84 19.03 58.60 51.39 59.50 55.78 63.22 29.18 33.13 67.16 31.48 44.62 111.85 115.38 73.32 72.45
3.325 17.31 18.42 58.40 50.96 59.31 55.25 62.79 29.25 33.30 66.12 30.50 44.09 111.69 114.77 72.64 71.78
BHandHLYP
2.825 20.14 21.65 56.79 51.09 57.91 55.98 62.78 25.33 29.25 69.93 37.32 46.54 105.24 111.02 73.12 72.35
2.925 19.10 20.50 56.51 50.34 57.64 55.06 62.00 25.49 29.55 67.98 35.25 45.67 105.10 110.06 72.05 71.23
3.025 18.19 19.50 56.23 49.67 57.37 54.25 61.30 25.61 29.82 66.32 33.49 44.88 104.91 109.18 71.09 70.25
3.125 17.43 18.65 55.97 49.09 57.09 53.54 60.70 25.71 30.04 64.91 32.02 44.18 104.70 108.40 70.24 69.40
3.225 16.80 17.94 55.72 48.59 56.84 52.91 60.18 25.79 30.23 63.72 30.78 43.57 104.49 107.71 69.49 68.66
3.325 16.29 17.35 55.50 48.17 56.60 52.36 59.75 25.85 30.39 62.74 29.76 43.04 104.30 107.12 68.85 68.02
Chapter 3 – Results and Discussion
68
A change in the chemical shift as a function of the interaction angle was also
observed. The change in angle yielded only small changes, on the order of less than 2 ppm
between 140° and 180°. Overall, as the angle gets closer to 180°, the chemical shift decreases.
The largest magnitude of change occurs between 140° and 160°, which could be explained
by the gradual approach of Y to the methyl hydrogens, introducing a C-H∙∙∙Y hydrogen bond,
and begins to slow down as the angle approaches 180° as the tetrel bond becomes dominant.
It is clear then that the tetrel bond distance remains the dominant effect on the carbon
chemical shift and consequently, any effect of the angle on the chemical shift is expected to
be negligible or overshadowed by other effects.
In additional to chemical shifts and energy, J-couplings are valuable parameters for
the characterization of noncovalent interactions. Trans-hydrogen bond J-coupling has been
studied extensively as an important tool for obtaining direct experimental evidence of
hydrogen bonding via NMR.138,139,140,141,142,143,144 Recently, computed J-coupling constants
have been reported for a series of noncovalent interactions, including pnicogen bonding,
chalcogen bonding and halogen bonding.145,146,43 For instance, in a recent study by Del Bene
et al., the interaction distance in a P-P pnicogen bond is estimated by the calculated
correlation between the J-coupling and the interaction distance.146 As such, J-coupling could
provide a valuable probe of tetrel bonds.
In the present study, J-coupling was calculated for each of the model compounds
(Figure 14) using the LC-PBE-D3, BHandHLYP, and CAM-B3LYP functionals. Total
1cJ(13C,17O/15N) coupling constants across the carbon tetrel bond are plotted in Figure 18 as
a function of the interaction distance in order to gain information as to whether the J-coupling
Chapter 3 – Results and Discussion
69
can provide evidence for the presence of the carbon tetrel bond. Here, we propose use of the
“1cJ” nomenclature to denote trans-carbon bond coupling, in analogy with the “1hJ, 2hJ” etc.
labels used in the literature for trans-hydrogen bond couplings. In each case, the roles of the
Fermi contact (FC), spin-dipolar (SD), paramagnetic spin-orbital (PSO), and diamagnetic
spin-orbital (DSO) mechanisms were assessed to evaluate their contributions to the total J-
coupling (Table 6 to Table 8, Appendix I – Supplementary Data). In all of the model
structures, the FC mechanism contributes 100% ± 5% of the total, suggesting an overlap of
orbitals with spin density centered at the nuclei of the carbon and the oxygen or nitrogen
atoms. The importance of various coupling mechanisms in different models suggests a
delicate interplay between these mechanisms147 depending on the exact geometrical details
and charge state of the model.
It can be observed in all cases that the coupling value (1cJ(13C,17O) or 1cJ(13C,15N))
becomes more negative as the interaction distance becomes shorter. Clearly there exists a
correlation between interaction distance and the magnitude of 1cJ, thereby providing a new
parameter for the study of carbon tetrel bonds. In each case, a second-order polynomial fits
the data with a correlation coefficient, R2, of at least 0.99 (Table 9-Table 11, Appendix I).
The data corroborate the findings for pnicogen and halogen bonding as well, where
analogous correlations have also been observed computationally. In one case of pnicogen
bonding, J(31P,31P) decreases from hundreds of hertz toward zero as the interaction distance
is increased. 146 In the case of J-coupling across Cl···N halogen bonds, computations show
that the J(35/37Cl,15N) value approaches 0 Hz from values of between approximately -60 and
-90 Hz, as the interaction distance is increased. 70
Chapter 3 – Results and Discussion
70
Figure 18. Computed J-coupling for model compounds. Graphs represent 1cJ-coupling
values between 13C and either 17O or 15N using (a) The LC-PBE-D3, (b) BHandHLYP, and
(c) CAM-B3LYP methods. In each case, the 6-311++G(d,p) basis set is used. Each plot is fit
by a quadratic polynomial function with R2 > 0.99 (Table 9 to Table 11 in Appendix I –
Supplementary Data).
3.2 Experimental NMR Investigations of Noncovalent Tetrel Bonds
The calculations on isolated model systems provide valuable insight into the
relationship between NMR parameters and tetrel bonds. Given that the crystal lattice can
influence NMR parameters, a further step was taken in order to investigate dependence of
carbon chemical shift on the carbon tetrel bond in the case of crystal structures. The CSD
was used to search for published crystal structures that contain carbon tetrel bonds. Because
there is not yet a universally accepted definition of a tetrel bond, candidate compounds were
screened for using two criteria, which are in accordance with the IUPAC standard for halogen
bonds: (1) The C···Y interaction distance must be within the sum of their van der Waals radii
and (2) R-C···Y angle must be within 160° and 180°.148 We note that these criteria are
Chapter 3 – Results and Discussion
71
slightly stricter than those used in the work of Thomas and co-workers, wherein the angle
range used is 140° to 180°.58 Among a large number of hits were sarcosinium tartrate (dC...O
= 3.08 Å) (Figure 6), sarcosine maleate (dC...O = 2.96 Å), and N,N,N’,N’-
tetramethylethylenediammonium succinate succinic acid (dC...O = 3.07 Å) (Figure 19) which
were found to be good carbon tetrel-bonding candidates for this study.44,149 Each salt is
compared to its corresponding salt lacking a tetrel bond.
Figure 19. The tetrel bond present in N,N,N’,N’-tetramethylethylenediammonium succinate
succinic acid. The interaction distance is 3.07 Å.
Although the tetrel bonds in these compounds are significant on the basis of the C…O
distances, there was concern with respect to the possible impact of competing weak C-H…O
hydrogen bonds. In the case of sarcosinium tartrate, the distances between O and H are
greater than 2.72 Å, the sum of their vdW radii. In sarcosinium maleate, there is a single
hydrogen 2.70 Å from the oxygen, according to the published crystal structure. Thus, for
Chapter 3 – Results and Discussion
72
these two salts, the strengths of the tetrel bonds, as judged by the reduced distance parameter
(RX···Y; eqn. 36) are significant whereas the strength of hydrogen bonds as quantified by the
same criteria is far less important. Generally, the methyl protons are splayed with respect to
the oxygen. The possible role of trifurcated hydrogen bonds in such systems has been
discussed in ref 58. In the case of N,N,N’,N’-tetramethylethylenediammonium succinate
succinic acid, there are not competing hydrogen bonds directly with the tetrel bonded oxygen
atom, however, the methyl hydrogens still make close contacts with other oxygen atoms in
the system. Regardless of the possible weak influence of a weak trifurcated hydrogen bond,
the presence of a tetrel bond means that de facto this interaction contributes to the observed
chemical shift.
The compounds were first made according to the literature sources (See section 2.4.1).
PXRD was used to confirm the identities of the substances. The PXRD show good agreement
between the obtained compounds and the simulated source. In the case of sarcosine, there is
only an extra peak at about 26o, but one peak missing at about 33o on the 2𝜃 axis (Figure
20), while sarcosinium tartrate shows almost perfect agreement with the simulated
diffraction patters, albeit with stronger signal intensities (Figure 21). The N,N,N’,N’-
tetramethylethylenediammonium salts are shown to have good agreement with their
simulated diffraction patterns (Figure 22 and Figure 23).
Chapter 3 – Results and Discussion
73
Figure 20. Powder X-Ray diffractogram of sarcosine. The simulated diffractogram (a) was
obtained using the Mercury version 3.5.1 software provided by the CCDC. The experimental
diffractogram (b) was obtained from a powdered sample using a Rigaku Ultima IV X-ray
diffractometer.
Chapter 3 – Results and Discussion
74
Figure 21. Powder X-Ray diffractogram of sarcosinium tartrate. The simulated
diffractogram (a) was obtained using the Mercury version 3.5.1 software provided by the
CCDC. The experimental diffractogram (b) was obtained from a powdered sample using a
Rigaku Ultima IV X-ray diffractometer.
Chapter 3 – Results and Discussion
75
Figure 22. Powder X-Ray diffractogram of N,N,N’,N’-tetramethylethylenediammonium
dichloride. The simulated diffractogram (a) was obtained using the Mercury version 3.5.1
software provided by the CCDC. The experimental diffractogram (b) was obtained from a
powdered sample using a Rigaku Ultima IV X-ray diffractometer.
a
b
Chapter 3 – Results and Discussion
76
Figure 23. Powder X-Ray diffractogram of N,N,N’,N’-tetramethylethylenediammonium
succinate succinic acid. The simulated diffractogram (a) was obtained using the Mercury
version 3.5.1 software provided by the CCDC. The experimental diffractogram (b) was
obtained from a powdered sample using a Rigaku Ultima IV X-ray diffractometer.
The GIPAW DFT computed and experimental 13C solid state NMR chemical shifts
corresponding the sarcosine and N,N,N’,N’-tetramethylethylenediammonium methyl groups
a
b
Chapter 3 – Results and Discussion
77
(Figure 24 to Figure 27) involved in the both in the presence of a carbon tetrel bond and in
the absence are reported in Table 5. In the same table, the C…O noncovalent bond distances,
as well as the N-C covalent bond distances are obtained from the CSD.
Figure 24. 13C CP/MAS spectra of sarcosine (top) and sarcosinium tartrate (bottom).
Spinning sidebands are denoted with asterisks. 𝐵0 = 9.4 T.
Chapter 3 – Results and Discussion
78
Figure 25. Selected regions of experimental 13C cross-polarization magic-angle spinning
(CP/MAS) NMR spectra of the methyl carbon associated with a tetrel bond. 𝐵0 = 9.4 T. (a)
Sarcosinium Tartrate. (b) Sarcosine.
Chapter 3 – Results and Discussion
79
Figure 26. 13C CP/MAS spectra of N,N,N’,N’-tetramethylethylenediammonium dichloride
(top) and N,N,N’,N’-tetramethylethylenediammonium succinate succinic acid (bottom).
Spinning sidebands are denoted with asterisks. 𝐵0 = 9.4 T.
Chapter 3 – Results and Discussion
80
Figure 27. Selected regions of experimental 13C cross-polarization magic-angle spinning
(CP/MAS) NMR spectra of the methyl carbon associated with a tetrel bond. 𝐵0 = 9.4 T. (a)
N,N,N’,N’-tetramethylethylenediammonium dichloride. (b) N,N,N’,N’-
tetramethylethylenediammonium succinate succinic acid.
Chapter 3 – Results and Discussion
81
Table 5. Calculated GIPAW and experimental 13C isotropic chemical shifts for the methyl
carbon on sarcosine compounds.
compound
N-C
Bond
Length
/ Å
Interaction
Distance
(C…O)
/ Å
RC∙∙∙O
iso(13C)
calc.
/ ppm
calc.
/ppm
calc.
iso(13C)
exp.
/ ppm
Sarcosine 1.4813(3) n/a n/a 37.9 56.8 0.773 31.5
Sarcosinium Tartrate 1.485(3) 3.08 0.96 43.6 61.8 0.604 34.7
Sarcosinium Maleate 149 1.497(2) 2.96 0.92 47.9 55.0 0.753 36
TMEDAa HCl 1.487(4) n/a n/a 27.8 72.1 0.879 41.4
1.486(4) n/a n/a 32.0 86.8 0.635 46.0
TMEDAa succinate 1.493(2) 3.07 0.95 33.4 89.6 0.646 44.3
1.487(2) 3.26 1.01 31.4 73.3 0.898 46.2
(a) TMEDA refers to N,N,N’,N’-tetramethylethylenediammonium.
(b) Entries in bold correspond to the methyl carbons of interest. In TMEDA succinate, the bolded
entry participates in the -hole interaction, whereas the other methyl carbon does not.
It is interesting to note that in each of the cases where the carbon tetrel bond is present,
the introduction of this interaction causes the chemical shift of the methyl group to increase.
In addition, the N-C bond lengthens in the presence of the tetrel bond. These trends are
reflected in both the GIPAW calculations and the experimental results where the chemical
shift increases are on the order of 5 to 10 ppm and 3 to 5 ppm, respectively. The magnitudes
of the increases noted from solid-state NMR spectroscopy experiments mirror much more
closely the increases calculated for isolated model systems.
The trends predicted by the GIPAW calculations are nevertheless also consistent with
the experimental data. Note that a comparison of the experimental and calculated absolute
values of the chemical shifts, while perhaps providing some insight into the overall accuracy
Chapter 3 – Results and Discussion
82
of the computational method and absolute shielding scale used, does not detract from the
findings as far as the trend in the values as a function of the tetrel bond distance.
We note that in the cases of the sarcosine salts, the amine becomes protonated,
whereas sarcosine itself is neutral. We assessed the potential competing effect of this
protonation on the methylamine 13C chemical shift and found there to be a slight difference
between the neutral and charged molecules. In a literature review, it was noted that the effect
of protonation of sarcosine causes a decrease in the methylamine 13C chemical shift by 1.83
ppm, from 35.75 ppm to 33.92 ppm (in solution where the carboxylate is negatively charged).
150 This trend was confirmed by Batchelor and co-workers, who noted that the 13C
protonation shift of a methylamine is -2.04 ppm 151, while Thursfield and coworkers
distinguish a chemical shift difference of about -2.7 ppm between monomethylamine (=
26.9 to 27.5 ppm) and the corresponding cation (= 24.3 to 24.8 ppm) during a conversion
of methanol and ammonia over the zeolite H-SAPO-34. 152 Thursfield’s results are also
confirmed by Jiang et al. 153 Given these experimental results reported in the literature,
protonation of the amine in sarcosine would therefore be expected to produce a small
negative change in the chemical shift, on the order of 2 to 3 ppm. However, our experimental
and computational data present a change in chemical shift in the opposite direction upon the
combined introduction of a tetrel bond and amine protonation. Therefore, this strongly
suggests that the dominant cause for this change is the introduction of the carbon tetrel bond.
Chapter 4 – Conclusions
83
Chapter 4 - Conclusions
This combined computational and experimental work has provided several outcomes
and insights into the nature of tetrel bonding. First, the quantum chemical calculations on
isolated model systems show that the chemical shifts of carbon atoms acting as tetrel bond
donors increase with the strength of the interaction. Both diamagnetic and paramagnetic
contributions to the magnetic shielding constant are responsible for this trend. Furthermore,
13C chemical shift anisotropies increase with the strength of the interaction.
In agreement with the computations on isolated models, calculations using periodic
boundary conditions to model the effects of an infinite crystal lattice (GIPAW DFT) show
that the chemical shifts of carbon atoms acting as tetrel bond donors increase relative to
parent compounds where tetrel bonds are absent. Experimental data for sarcosine, where no
tetrel bond is present, and for two sarcosine salts exhibiting tetrel bonds in the solid state
confirm the computational trends described by both the cluster model analysis as well as the
GIPAW DFT calculations on published crystal structures.
Cluster model calculations of trans-tetrel bond J couplings show that the magnitude
of 1cJ(13C,17O) increases from zero to several hertz as the C…O interaction distance is
decreased to less than the sum of their van der Waals radii. The couplings are typically, but
not always, entirely due to the Fermi-contact coupling mechanism.
In summary, the present work provides compelling computational and experimental
evidence that the carbon tetrel bond has an influence on NMR parameters in the solid state,
thus creating opportunities to use NMR crystallography to characterize tetrel-bonded
supramolecular architectures and functional materials.
Chapter 4 – Conclusions
84
There is still work to be done in completing the characterization of the carbon tetrel
bond. Concurrently, there is an opportunity for further study of other tetrel elements in order
to understand the nature of the electronic structures of these bonds. Further research
involving silicon, germanium, tin, and lead would be useful using both SSNMR methods and
ab initio computational studies using our state-of-the-art equipment at the National
Ultrahigh-Field NMR Facility for Solids. The crystal structures will first be solved by X-ray
diffraction, and the study of these nuclides by multinuclear SSNMR will provide key data
relevant to this project. The chemical shift response as a result of the formation of the tetrel
bond, as well as other NMR parameters, will assist in developing a clear picture of the tetrel
bond. Quantum calculations using density functional theory at the Canadian High
Performance Computing Virtual Laboratory will be used to complement the experimental
data and confirm any observations.
85
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Appendix I – Supplementary Data
103
Appendix I – Supplementary Data
Table 6. Raw data obtained from calculations (BHandHLYP/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz.
Model
Structure
Interaction Distance
/Å FC SD PSO DSO Total J %FC
1
2.825 -5.7774400 -0.0033046 0.2211940 -0.0384239 -5.5979800 103.21
2.925 -4.4712100 -0.0046878 0.1923000 -0.0361786 -4.3197800 103.51
3.025 -3.4094900 -0.0053476 0.1677860 -0.0341417 -3.2811900 103.91
3.125 -2.6226900 -0.0055014 0.1470290 -0.0322869 -2.5134500 104.35
3.225 -1.9885400 -0.0053855 0.1294620 -0.0305911 -1.8950500 104.93
3.325 -1.4673700 -0.0051835 0.1145940 -0.0290354 -1.3870000 105.79
2
2.825 -5.9705500 -0.0078246 0.1891870 -0.0452860 -5.8344800 102.33
2.925 -4.6327300 -0.0069752 0.1657100 -0.0427530 -4.5167500 102.57
3.025 -3.5428000 -0.0061207 0.1452890 -0.0404468 -3.4440800 102.87
3.125 -2.7252700 -0.0052762 0.1276690 -0.0383392 -2.6412200 103.18
3.225 -2.0759500 -0.0045096 0.1125460 -0.0364059 -2.0043200 103.57
3.325 -1.5376900 -0.0039040 0.0996200 -0.0346266 -1.4766000 104.14
3
2.825 -8.4040300 -0.0281782 0.1026520 -0.0426263 -8.3721800 100.38
2.925 -6.5924800 -0.0231170 0.0990098 -0.0401181 -6.5567000 100.55
3.025 -5.1447500 -0.0190264 0.0943790 -0.0378430 -5.1072400 100.73
3.125 -3.9759900 -0.0157842 0.0892440 -0.0357710 -3.9383000 100.96
3.225 -3.0596900 -0.0131830 0.0839403 -0.0338769 -3.0228100 101.22
3.325 -2.3299300 -0.0111324 0.0786916 -0.0321394 -2.2945100 101.54
4
2.825 -6.8198200 -0.0044630 0.1741670 -0.0416687 -6.6917800 101.91
2.925 -5.3073500 -0.0047536 0.1525780 -0.0392216 -5.1987400 102.09
3.025 -4.0825800 -0.0046334 0.1342270 -0.0370014 -3.9899800 102.32
3.125 -3.1550400 -0.0042736 0.1186300 -0.0349796 -3.0756700 102.58
3.225 -2.4098300 -0.0037883 0.1053690 -0.0331312 -2.3413800 102.92
3.325 -1.7981900 -0.0033615 0.0940816 -0.0314359 -1.7389100 103.41
5
2.825 -9.8252900 -0.0168635 0.0579256 -0.0483889 -9.8326100 99.93
2.925 -7.7046100 -0.0132438 0.0628782 -0.0457005 -7.7006800 100.05
3.025 -6.0094900 -0.0105396 0.0647445 -0.0432492 -5.9985400 100.18
3.125 -4.6638700 -0.0085171 0.0645585 -0.0410055 -4.6488400 100.32
3.225 -3.5875200 -0.0070535 0.0630627 -0.0389446 -3.5704500 100.48
3.325 -2.7701800 -0.0058979 0.0607799 -0.0370452 -2.7523400 100.65
6
2.825 -9.9455000 -0.0232848 0.0420864 -0.0432029 -9.9699000 99.76
2.925 -7.8446900 -0.0165779 0.0470122 -0.0407596 -7.8550200 99.87
3.025 -6.1444700 -0.0115388 0.0484756 -0.0385370 -6.1460700 99.97
Appendix I – Supplementary Data
104
3.125 -4.7858100 -0.0077824 0.0477239 -0.0365071 -4.7823800 100.07
3.225 -3.7199100 -0.0050022 0.0456410 -0.0346461 -3.7139200 100.16
3.325 -2.8793500 -0.0029973 0.0428363 -0.0329341 -2.8724500 100.24
7
2.825 -6.6463000 -0.0044124 0.1966320 -0.0454815 -6.4995600 102.26
2.925 -5.1631800 -0.0053627 0.1717160 -0.0428884 -5.0397200 102.45
3.025 -3.9694600 -0.0056746 0.1507090 -0.0405297 -3.8649600 102.70
3.125 -3.0572400 -0.0055989 0.1329750 -0.0383764 -2.9682400 103.00
3.225 -2.3201700 -0.0053059 0.1179810 -0.0364033 -2.2439000 103.40
3.325 -1.7354800 -0.0049659 0.1052800 -0.0345894 -1.6697600 103.94
8
2.825 -0.1271800 0.0361270 0.0242229 -0.0618174 -0.1286480 98.86
2.925 -0.0054982 0.0319578 0.0221303 -0.0566491 -0.0080593 68.22
3.025 0.0631498 0.0283092 0.0202108 -0.0520746 0.0595952 105.96
3.125 0.1003810 0.0251565 0.0185288 -0.0480110 0.0960552 104.50
3.225 0.1167330 0.0224498 0.0170902 -0.0443888 0.1118850 104.33
3.325 0.1160610 0.0201338 0.0158772 -0.0411491 0.1109230 104.63
9
2.825 -4.2597800 0.0225266 -0.0167204 -0.0587748 -4.3127500 98.77
2.925 -3.3080100 0.0235869 -0.0086157 -0.0546399 -3.3476700 98.82
3.025 -2.5653100 0.0236232 -0.0031007 -0.0509301 -2.5957100 98.83
3.125 -1.9577100 0.0229638 0.0006016 0.0006016 -1.9817400 98.79
3.225 -1.4938800 0.0219128 0.0030470 -0.0445719 -1.5135000 98.70
3.325 -1.1350300 0.0206610 0.0046335 -0.0418364 -1.1515700 98.56
10
2.825 -6.0983126 0.0017227 0.0050878 -0.0329137 -6.1244174 99.57
2.925 -4.9026536 0.0013808 0.0072425 -0.0310196 -4.9250411 99.55
3.025 -3.9133502 0.0011910 0.0082917 -0.0292960 -3.9331708 99.50
3.125 -3.1038207 0.0010870 0.0086249 -0.0277219 -3.1218317 99.42
3.225 -2.4422932 0.0010361 0.0085185 -0.0262793 -2.4590137 99.32
3.325 -1.9123558 0.0010064 0.0081643 -0.0249530 -1.9281365 99.18
11
2.825 -7.2071145 -0.0094666 0.0007135 -0.0331168 -7.2489860 99.42
2.925 -5.7420051 -0.0097103 0.0041096 -0.0313214 -5.7789250 99.36
3.025 -4.5406510 -0.0095844 0.0060870 -0.0296808 -4.5738396 99.27
3.125 -3.5653329 -0.0346615 0.0071027 -0.0281762 -3.5956599 99.16
3.225 -2.7938314 -0.0087708 0.0074845 -0.0267919 -2.8219140 99.00
3.325 -2.1646509 -0.0082427 0.0074672 -0.0255144 -2.1909380 98.80
12
2.825 -10.0660045 -0.0078429 -0.0085749 -0.0343485 -10.1167693 99.50
2.925 -8.1384291 -0.0081146 -0.0036897 -0.0324641 -8.1826852 99.46
3.025 -6.5352910 -0.0081154 -0.0003020 -0.0307434 -6.5744412 99.40
3.125 -5.2075650 -0.0079637 0.0019808 -0.0291667 -5.2427174 99.33
3.225 -4.1433839 -0.0076689 0.0034615 -0.0277172 -4.1753100 99.24
3.325 -3.2698338 -0.0073289 0.0043746 -0.0263804 -3.2991789 99.11
13
2.825 -8.1897100 -0.0169981 0.1368380 -0.0484516 -8.1183300 100.88
2.925 -6.3826800 -0.0157425 0.1239260 -0.0456354 -6.3201300 100.99
3.025 -4.9396400 -4.9396400 0.1126660 -0.0430766 -4.8843300 101.13
Appendix I – Supplementary Data
105
3.125 -3.8350900 -0.0127527 0.1027790 -0.0407428 -3.7858100 101.30
3.225 -2.9168100 -0.0113448 0.0940566 -0.0386065 -2.8727000 101.54
3.325 -2.1867600 -0.0101220 0.0863351 -0.0366446 -2.1471900 101.84
14
2.825 -8.5663459 -0.0077326 0.0062075 -0.0357135 -8.6035743 99.57
2.925 -6.9161603 -0.0089168 0.0062827 -0.0337083 -6.9525050 99.48
3.025 -5.5426070 -0.0094103 0.0062205 -0.0318789 -5.5776753 99.37
3.125 -4.3996486 -0.0094761 0.0060534 -0.0302040 -4.4332861 99.24
3.225 -3.4964308 -0.0092233 0.0058142 -0.0286656 -3.5285112 99.09
3.325 -2.7531803 -0.0088270 0.0055360 -0.0272486 -2.7837317 98.90
15
2.825 -9.3865782 -0.0086330 0.0116579 -0.0359643 -9.4195283 99.65
2.925 -7.6781092 -0.0087286 0.0128835 -0.0339973 -7.7079593 99.61
3.025 -6.2383752 -0.0085638 0.0133839 -0.0322006 -6.2657564 99.56
3.125 -5.0195290 -0.0082747 0.0133938 -0.0305540 -5.0449605 99.50
3.225 -4.0311234 -0.0078702 0.0130872 -0.0290397 -4.0549417 99.41
3.325 -3.2214115 -0.0074234 0.0125935 -0.0276429 -3.2438833 99.31
16
2.825 -8.8206187 -0.0098034 0.0101711 -0.0340361 -8.8542983 99.62
2.925 -7.1904781 -0.0100231 0.0109761 -0.0321483 -7.2216749 99.57
3.025 -5.8218064 -0.0098948 0.0112125 -0.0304252 -5.8509131 99.50
3.125 -4.6605283 -0.0095923 0.0110726 -0.0288471 -4.6878956 99.42
3.225 -3.7354560 -0.0091251 0.0106975 -0.0273967 -3.7612802 99.31
3.325 -2.9739700 -0.0086028 0.0101924 -0.0260599 -2.9984336 99.18
Appendix I – Supplementary Data
106
Table 7. Raw data obtained from calculations (LC-PBE-D3/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz.
Model
Structure
Interaction Distance
/Å FC SD PSO DSO Total J %FC
1
2.825 -5.7930600 0.0005746 0.2305720 -0.0378695 -5.5997800 103.45
2.925 -4.4339900 -0.0015727 0.1988320 -0.0356548 -4.2723800 103.78
3.025 -3.3752800 -0.0027946 0.1723260 -0.0336477 -3.2393900 104.19
3.125 -2.5495100 -0.0034511 0.1501720 -0.0318206 -2.4346100 104.72
3.225 -1.9178000 -0.0037408 0.1316800 -0.0301513 -1.8200100 105.37
3.325 -1.4341400 -0.0038239 0.1162390 -0.0286203 -1.3503400 106.21
2
2.825 -6.0089700 -0.0039513 0.1973090 -0.0446880 -5.8603000 102.54
2.925 -4.6076600 -0.0041334 0.1710760 -0.0421888 -4.4829000 102.78
3.025 -3.5145100 -0.0040177 0.1487570 -0.0399152 -3.4096900 103.07
3.125 -2.6592700 -0.0037775 0.1298370 -0.0378379 -2.5710500 103.43
3.225 -2.0049800 -0.0034803 0.1138820 -0.0359334 -1.9305100 103.86
3.325 -1.5022400 -0.0031926 0.1004780 -0.0341809 -1.4391400 104.38
3
2.825 -8.0576200 -0.0185941 0.1264120 -0.0420964 -7.9918900 100.82
2.925 -6.2217000 -0.0154347 0.1174050 -0.0396212 -6.1593500 101.01
3.025 -4.7801800 -0.0128509 0.1086360 -0.0373767 -4.7217700 101.24
3.125 -3.6555100 -0.0107681 0.1003280 -0.0353333 -3.6012800 101.51
3.225 -2.7776700 -0.0091113 0.0926012 -0.0334664 -2.7276500 101.83
3.325 -2.0962600 -0.0077884 0.0855118 -0.0317541 -2.0503000 102.24
4
2.825 -5.7844300 0.0047817 0.0188364 -0.0397117 -5.8005200 99.72
2.925 -4.4449100 0.0082895 0.0222445 -0.0372518 -4.4516300 99.85
3.025 -3.3955600 0.0105454 0.0235193 -0.0350296 -3.3965200 99.97
3.125 -2.5780700 0.0118609 0.0234633 -0.0330136 -2.5757600 100.09
3.225 -1.9454700 0.0124985 0.0226469 -0.0311780 -1.9415000 100.20
3.325 -1.4600600 0.0126354 0.0214541 -0.0295010 -1.4554700 100.32
5
2.825 -8.6371600 -0.0238427 0.0770242 -0.0486771 -8.6326500 100.05
2.925 -6.6935800 -0.0185794 0.0771373 -0.0459368 -6.6809600 100.19
3.025 -5.1581700 -0.0145455 0.0753837 -0.0434429 -5.1407700 100.34
3.125 -3.9584100 -0.0114704 0.0725040 -0.0411647 -3.9385400 100.50
3.225 -3.0268100 -0.0091289 0.0690134 -0.0390758 -3.0060000 100.69
3.325 -2.2919700 -0.0073697 0.0652748 -0.0371536 -2.2712100 100.91
6
2.825 -8.6341500 -0.0259481 0.0489777 -0.0426850 -8.6538100 99.77
2.925 -6.7649200 -0.0185392 0.0515617 -0.0402109 -6.7721100 99.89
3.025 -5.2718700 -0.0130305 0.0511891 -0.0379651 -5.2716700 100.00
3.125 -4.0920500 -0.0089577 0.0490449 -0.0359182 -4.0878800 100.10
3.225 -3.1649200 -0.0059782 0.0459344 -0.0340456 -3.1590100 100.19
3.325 -2.4350000 -0.0038355 0.0423882 -0.0323268 -2.4287700 100.26
Appendix I – Supplementary Data
107
7
2.825 -6.3439100 -0.0008079 0.1601130 -0.0446853 -6.2292900 101.84
2.925 -4.8702400 -0.0007546 0.1404440 -0.0421074 -4.7726600 102.04
3.025 -3.7187100 -0.0005144 0.1236560 -0.0397662 -3.6353400 102.29
3.125 -2.8191100 -0.0002304 0.1093600 -0.0376309 -2.7476100 102.60
3.225 -2.1278400 0.0000373 0.0972072 -0.0356767 -2.0662700 102.98
3.325 -1.5945700 0.0002389 0.0868906 -0.0338823 -1.5413200 103.45
8
2.825 -0.0065126 0.0424602 -0.0140986 -0.0606358 -0.0387867 16.79
2.925 0.0932412 0.0374877 -0.0125142 -0.0554818 0.0627329 148.63
3.025 0.1433280 0.0331336 -0.0112246 -0.0509129 0.1143240 125.37
3.125 0.1589070 0.0293612 -0.0100983 -0.0468571 0.1313130 121.01
3.225 0.1547720 0.0261089 -0.0090655 -0.0432445 0.1285710 120.38
3.325 0.1401710 0.0233153 -0.0081110 -0.0400161 0.1153590 121.51
9
2.825 -3.8412100 0.0218847 -0.0399006 -0.0573358 -3.9165600 98.08
2.925 -2.9196000 0.0231508 -0.0299731 -0.0532334 -2.9796600 97.98
3.025 -2.2028100 0.0233431 -0.0226304 -0.0495549 -2.2516500 97.83
3.125 -1.6537800 0.0228383 -0.0171975 -0.0462446 -1.6943800 97.60
3.225 -1.2342900 0.0218951 -0.0131471 -0.0432560 -1.2688000 97.28
3.325 -0.9143350 0.0206784 -0.0101024 -0.0405491 -0.9443080 96.83
10
2.825 -5.0430248 0.0112429 0.0012606 -0.0312384 -5.0617512 99.63
2.925 -3.9877650 0.0108981 0.0040728 -0.0293312 -4.0021290 99.64
3.025 -3.1304585 0.0104404 0.0056437 -0.0276050 -3.1419749 99.63
3.125 -2.4431769 0.0099019 0.0063992 -0.0260362 -2.4529119 99.60
3.225 -1.8972484 0.0093185 0.0066469 -0.0246053 -1.9058893 99.55
3.325 -1.4671574 0.0087180 0.0066010 -0.0232960 -1.4751389 99.46
11
2.825 -5.7626112 0.0081290 -0.0051309 -0.0318689 -5.7914934 99.50
2.925 -4.5365971 0.0078691 -0.0016199 -0.0300013 -4.5603594 99.48
3.025 -3.5495101 0.0075152 0.0005860 -0.0283064 -3.5697094 99.43
3.125 -2.7569817 0.0071012 0.0019020 -0.0267618 -2.7747402 99.36
3.225 -2.1339030 0.0066569 0.0026323 -0.0253497 -2.1499643 99.25
3.325 -1.6435928 0.0062063 0.0029931 -0.0240543 -1.6584477 99.10
12
2.825 -9.4753289 -0.0079882 -0.0035862 -0.0332475 -9.5201602 99.53
2.925 -7.5293777 -0.0088041 -0.0003627 -0.0314226 -7.5699727 99.46
3.025 -5.9442648 -0.0091312 0.0018270 -0.0297575 -5.9813249 99.38
3.125 -4.6686922 -0.0091330 0.0032552 -0.0282329 -4.7028066 99.27
3.225 -3.6511519 -0.0089259 0.0041419 -0.0268324 -3.6827554 99.14
3.325 -2.8424500 -0.0085870 0.0046485 -0.0255417 -2.8719354 98.97
13
2.825 -7.8771000 -0.0100444 0.1495560 -0.0475216 -7.7851100 101.18
2.925 -6.0514700 -0.0098800 0.1336920 -0.0447581 -5.9724100 101.32
3.025 -4.6218300 -0.0093202 0.1201630 -0.0422482 -4.5532400 101.51
3.125 -3.5144200 -0.0085856 0.1085420 -0.0399601 -3.4544200 101.74
3.225 -2.6609300 -0.0077988 0.0985066 -0.0378669 -2.6080900 102.03
3.325 -2.0001200 -0.0070462 0.0898050 -0.0359449 -1.9533100 102.40
Appendix I – Supplementary Data
108
14
2.825 -8.0504779 -0.0086993 0.0019223 -0.0351461 -8.0923915 99.48
2.925 -6.3727006 -0.0097991 0.0023905 -0.0331664 -6.4132675 99.37
3.025 -5.0120525 -0.0101808 0.0027250 -0.0313618 -5.0508660 99.23
3.125 -3.9226503 -0.0101107 0.0029358 -0.0297108 -3.9595421 99.07
3.225 -3.0599713 -0.0097701 0.0030532 -0.0281957 -3.0948853 98.87
3.325 -2.3747518 -0.0092785 0.0031025 -0.0268011 -2.4077299 98.63
15
2.825 -8.8160037 -0.0147454 -0.0083638 0.0112335 -8.8488136 99.63
2.925 -7.0870689 -0.0087491 0.0120321 -0.0337284 -7.1175081 99.57
3.025 -5.6569857 -0.0087716 0.0122744 -0.0319444 -5.6854330 99.50
3.125 -4.4917659 -0.0085585 0.0121476 -0.0303102 -4.5184879 99.41
3.225 -3.5477006 -0.0082177 0.0117955 -0.0288083 -3.5729357 99.29
3.325 -2.7903526 -0.0077974 0.0113178 -0.0274235 -2.8142551 99.15
16
2.825 -8.2436899 -0.0097808 0.0081368 -0.0337594 -8.2790948 99.57
2.925 -6.5982315 -0.0101530 0.0088711 -0.0318835 -6.6314061 99.50
3.025 -5.2452002 -0.0101079 0.0091352 -0.0301724 -5.2763408 99.41
3.125 -4.1488545 -0.0098008 0.0090849 -0.0286063 -4.1781856 99.30
3.225 -3.2638301 -0.0093544 0.0088430 -0.0271679 -3.2915059 99.16
3.325 -2.5570505 -0.0088253 0.0084941 -0.0258431 -2.5832255 98.99
Appendix I – Supplementary Data
109
Table 8. Raw data obtained from calculations (CAM-B3LYP/6-311++G(d,p)) of
1cJ(13C,17O/15N) in model structures. All values are reported in Hz.
Model
Structure
Interaction Distance
/Å FC SD PSO DSO Total J %FC
1
2.825 -6.2104200 0.0006354 0.2383710 -0.0378105 -6.0092200 103.35
2.925 -4.8158300 -0.0011225 0.2062680 -0.0356041 -4.6462900 103.65
3.025 -3.6902000 -0.0021042 0.1791590 -0.0336026 -3.5467500 104.04
3.125 -2.8359600 -0.0025646 0.1562930 -0.0317799 -2.7140200 104.49
3.225 -2.1588400 -0.0027119 0.1370110 -0.0301135 -2.0546500 105.07
3.325 -1.6102800 -0.0027199 0.1207470 -0.0285847 -1.5208400 105.88
2
2.825 -6.4276600 -0.0056128 0.2037530 -0.0446052 -6.2741200 102.45
2.925 -4.9976400 -0.0049976 0.1777020 -0.0421144 -4.8670500 102.68
3.025 -3.8414700 -0.0043257 0.1551460 -0.0398466 -3.7305000 102.97
3.125 -2.9557000 -0.0036523 0.1357460 -0.0377741 -2.8613800 103.30
3.225 -2.2586300 -0.0030270 0.1191450 -0.0358729 -2.1783800 103.68
3.325 -1.6914400 -0.0025173 0.1049920 -0.0341229 -1.6230900 104.21
3
2.825 -9.0551400 -0.0256854 0.1088650 -0.0419433 -9.0139000 100.46
2.925 -7.1200400 -0.0207014 0.1042500 -0.0394793 -7.0759700 100.62
3.025 -5.5681900 -0.0167037 0.0988112 -0.0372440 -5.5233300 100.81
3.125 -4.3144800 -0.0135585 0.0930015 -0.0352083 -4.2702400 101.04
3.225 -3.3335000 -0.0110549 0.0871303 -0.0333473 -3.2907700 101.30
3.325 -2.5535900 -0.0090947 0.0814030 -0.0316400 -2.5129200 101.62
4
2.825 -7.1509900 -0.0019952 0.1554770 -0.0408194 -7.0383300 101.60
2.925 -5.5707300 -0.0014109 0.1368530 -0.0384047 -5.4736900 101.77
3.025 -4.3104500 -0.0007735 0.1207300 -0.0362150 -4.2267100 101.98
3.125 -3.3226400 -0.0001830 0.1068230 -0.0342220 -3.2502300 102.23
3.225 -2.5426600 0.0003509 0.0948642 -0.0324011 -2.4798500 102.53
3.325 -1.9248700 0.0007476 0.0846023 -0.0307318 -1.8702500 102.92
5
2.825 -11.3519000 -0.0000491 0.0587627 -0.0469496 -11.3402000 100.10
2.925 -8.9184400 -0.0000178 0.0642715 -0.0443818 -8.8985700 100.22
3.025 -6.9600600 -0.0001478 0.0664115 -0.0420362 -6.9358300 100.35
3.125 -5.4113300 -0.0003671 0.0663145 -0.0398857 -5.3852700 100.48
3.225 -4.1959700 -0.0005823 0.0647892 -0.0379071 -4.1696700 100.63
3.325 -3.2160800 -0.0008257 0.0624041 -0.0360810 -3.1905800 100.80
6
2.825 -11.0661000 -0.0140711 0.0547235 -0.1367140 -11.0675000 99.99
2.925 -8.7333600 -0.0095469 0.0582667 -0.0397536 -8.7243900 100.10
3.025 -6.8520700 -0.0061800 0.0584133 -0.0376087 -6.8374400 100.21
3.125 -5.3524900 -0.0037196 0.0564311 -0.0356474 -5.3354200 100.32
3.225 -4.1732400 -0.0019123 0.0532124 -0.0338471 -4.1557800 100.42
3.325 -3.2355700 -0.0006361 0.0493699 -0.0321893 -3.2190200 100.51
Appendix I – Supplementary Data
110
7
2.825 -7.1771300 -0.0009220 0.2193690 -0.0448664 -7.0035500 102.48
2.925 -5.5848300 -0.0025383 0.1904710 -0.0423171 -5.4392200 102.68
3.025 -4.2988900 -0.0033561 0.1662810 -0.0399979 -4.1759700 102.94
3.125 -3.3196100 -0.0036502 0.1459850 -0.0378803 -3.2151500 103.25
3.225 -2.5300200 -0.0036433 0.1289110 -0.0359396 -2.4407000 103.66
3.325 -1.8971400 -0.0035336 0.1145110 -0.0341552 -1.8203200 104.22
8
2.825 -0.1206650 0.0298742 0.0218952 -0.0610709 -0.1299660 92.84
2.925 0.0040753 0.0264024 0.0202067 0.0525804 0.0049529 82.28
3.025 0.0732845 0.0233542 0.0186079 -0.0514273 0.0638193 114.83
3.125 0.1084270 0.0207182 0.0171776 -0.0474058 0.0989171 109.61
3.225 0.1225330 0.0184569 0.0159364 -0.0438214 0.1131050 108.34
3.325 0.1202560 0.0165275 0.0148781 -0.0406157 0.1110460 108.29
9
2.825 -4.5047000 0.0174908 -0.0294744 -0.0576875 -4.5743700 98.48
2.925 -3.4852900 0.0192342 -0.0194277 -0.0536179 -3.5391100 98.48
3.025 -2.6966300 0.0198243 -0.0122374 -0.0499668 -2.7390100 98.45
3.125 -2.0582200 0.0196516 -0.0071149 -0.0466796 -2.0923600 98.37
3.225 -1.5614900 0.0190038 -0.0034815 -0.0437098 -1.5896700 98.23
3.325 -1.1932200 0.0180825 -0.0009137 -0.0410180 -1.2170700 98.04
10
2.825 -6.40650637 0.003593 0.0012969 -0.0324108 -6.43402794 99.57
2.925 -5.15837125 0.0031398 0.0041538 -0.0305393 -5.18161448 99.55
3.025 -4.12193613 0.0028182 0.0057513 -0.0288368 -4.14219155 99.51
3.125 -3.27551482 0.0025756 0.0065112 -0.0272824 -3.29370823 99.45
3.225 -2.5834359 0.0023894 0.0067366 -0.0258583 -2.60017046 99.36
3.325 -2.02571045 0.002235 0.006641 -0.0245496 -2.04137894 99.23
11
2.825 -7.03722989 0.0016791 -0.0087616 -0.0323207 -7.07663258 99.44
2.925 -5.62066897 0.0012662 -0.0039705 -0.0305045 -5.65387159 99.41
3.025 -4.46000809 0.0009776 -0.0008647 -0.0288497 -4.48875003 99.36
3.125 -3.51733145 0.0007717 0.001067 -0.0273364 -3.54283308 99.28
3.225 -2.76022196 0.0006309 0.0021991 -0.0259478 -2.78333895 99.17
3.325 -2.1518299 0.0005283 0.0028024 -0.02467 -2.17316543 99.02
12
2.825 -10.8649434 -0.0052768 -0.0150692 -0.0339372 -10.919215 99.50
2.925 -8.81169737 -0.0057432 -0.0091936 -0.0320781 -8.85871688 99.47
3.025 -7.10437858 -0.0059399 -0.0050001 -0.0303803 -7.145703 99.42
3.125 -5.68628868 -0.0059786 -0.0020591 -0.0288248 -5.72315243 99.36
3.225 -4.53797182 -0.0058756 -3.86E-05 -0.0273948 -4.57128666 99.27
3.325 -3.60076583 -0.0056974 0.0013184 -0.0260759 -3.6312191 99.16
13
2.825 -8.7675500 -0.0129312 0.1443740 -0.0475191 -8.6836200 100.97
2.925 -6.8426300 -0.0119873 0.1298540 -0.0447587 -6.7695300 101.08
3.025 -5.3049300 -0.0108222 0.1173480 -0.0422508 -5.2406600 101.23
3.125 -4.1119300 -0.0095903 0.1064880 -0.0399636 -4.0550000 101.40
3.225 -3.1414500 -0.0084381 0.0970003 -0.0378700 -3.0907600 101.64
3.325 -2.3753500 -0.0074290 0.0886742 -0.0359474 -2.3300500 101.94
Appendix I – Supplementary Data
111
14
2.825 -9.0404265 -0.0068039 -0.0018878 -0.0350812 -9.0842057 99.52
2.925 -7.3035242 -0.0078135 -0.0004817 -0.0331109 -7.3449327 99.44
3.025 -5.8600168 -0.0082183 0.0005164 -0.0313136 -5.8990407 99.34
3.125 -4.6634180 -0.0082495 0.0011968 -0.0296683 -4.7001414 99.22
3.225 -3.7051991 -0.0080141 0.0016384 -0.0281574 -3.7397343 99.08
3.325 -2.9226160 -0.0076477 0.0019098 -0.0267659 -2.9551173 98.90
15
2.825 -10.0110455 -0.0074487 0.0056522 -0.0354680 -10.0483161 99.63
2.925 -8.2127036 -0.0075159 0.0079111 -0.0335297 -8.2458361 99.60
3.025 -6.6946271 -0.0073663 0.0092236 -0.0317595 -6.7245193 99.56
3.125 -5.4119427 -0.0071100 0.0098740 -0.0301371 -5.4393100 99.50
3.225 -4.3603441 -0.0067643 0.0100748 -0.0286451 -4.3856774 99.42
3.325 -3.4965009 -0.0063814 0.0099850 -0.0272689 -3.5201650 99.33
16
2.825 -9.3518606 -0.0082658 0.0034613 -0.0335584 -9.3902253 99.59
2.925 -7.6401092 -0.0084667 0.0053658 -0.0316985 -7.6749109 99.55
3.025 -6.2019463 -0.0083684 0.0064717 -0.0300009 -6.2338443 99.49
3.125 -4.9872101 -0.0081144 0.0070226 -0.0284462 -5.0167376 99.41
3.225 -4.0040086 -0.0077290 0.0072001 -0.0270176 -4.0315442 99.32
3.325 -3.1970882 -0.0072891 0.0071397 -0.0257008 -3.2229405 99.20
Table 9. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(BHandHLYP/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
iso
/ ppm
Model A B C R2
1 -9.88 69.06 -121.84 0.9995
2 -10.17 71.13 -125.62 0.9996
3 -13.52 95.20 -169.38 0.9998
4 -11.34 79.53 -140.83 0.9996
5 -16.19 113.58 -201.50 0.9998
6 -15.94 112.14 -199.48 0.9998
7 -11.13 77.97 -137.96 0.9997
8 -1.46 9.41 -15.08 0.9941
9 -7.41 51.85 -91.61 0.9998
10 -8.32 59.50 -107.81 0.9999
11 -10.57 75.06 -134.91 0.9999
12 -13.31 95.41 -173.40 0.9999
13 -13.31 93.66 -166.45 0.9996
14 -11.45 81.99 -148.84 0.9999
15 -11.27 81.61 -150.02 1.0000
Appendix I – Supplementary Data
112
16 -10.94 78.93 -144.54 1.0000
Table 10. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(LC-PBE-D3/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
iso
/ ppm
Model A B C R2
1 -10.65 73.88 -129.32 0.9997
2 -11.00 76.40 -133.87 0.9997
3 -14.34 99.96 -175.87 0.9997
4 -10.71 74.46 -130.65 0.9997
5 -15.21 106.10 -186.97 0.9997
6 -14.36 100.66 -178.37 0.9998
7 -11.58 80.46 -141.12 0.9997
8 -1.41 8.97 -14.09 0.9849
9 -7.63 52.78 -92.14 0.9996
10 -7.85 55.40 -98.91 0.9998
11 -9.22 64.88 -115.51 0.9998
12 -14.23 100.74 -180.47 0.9999
13 -14.43 100.28 -175.87 0.9997
14 -12.41 87.61 -156.52 0.9998
15 -12.16 86.77 -156.92 0.9999
16 -11.73 83.47 -150.43 0.9999
Appendix I – Supplementary Data
113
Table 11. Polynomial fit information for 1cJ(13C,17O/15N) vs the carbon tetrel bond length
(CAM-B3LYP/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
iso
/ ppm
Model A B C R2
1 -10.55 73.73 -130.11 0.9996
2 -10.84 75.89 -134.10 0.9997
3 -14.45 101.77 -181.15 0.9998
4 -11.93 83.61 -147.98 0.9997
5 -18.40 129.27 -229.68 0.9998
6 -17.61 123.85 -220.38 0.9998
7 -11.92 83.55 -147.89 0.9996
8 -1.54 9.93 -15.87 0.9861
9 -8.04 56.10 -98.88 0.9998
10 -8.66 62.01 -112.46 0.9999
11 -10.15 72.17 -129.93 0.9999
12 -14.01 100.67 -183.46 0.9999
13 -14.33 100.70 -178.77 0.9997
14 -11.99 85.94 -156.14 0.9999
15 -11.71 85.00 -156.72 1.0000
16 -11.35 82.10 -150.70 1.0000
Appendix I – Supplementary Data
114
Table 12. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (MP2/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 6.45 -42.81 71.12 0.9977 8.03 -57.07 98.07 0.9999
2 6.45 -42.71 70.68 0.9976 7.94 -56.63 97.63 0.9999
3 3.18 -17.27 14.43 0.9981 2.79 -20.61 59.49 1.0000
4 5.61 -36.78 59.84 0.9970 6.06 -43.39 96.62 0.9999
5 2.77 -13.61 4.74 0.9988 2.53 -19.03 57.35 1.0000
6 5.86 -37.00 54.96 0.9841 4.36 -32.79 81.43 1.0000
7 5.61 -36.84 60.07 0.9968 6.67 -47.72 114.32 0.9999
8 16.96 -112.74 185.57 0.9985 0.18 -1.65 117.48 1.0000
9 5.11 -31.55 45.58 0.9602 0.46 -4.03 106.67 0.9999
10 8.21 -54.40 89.68 0.9977 7.29 -53.12 124.51 1.0000
11 7.86 -51.93 85.01 0.9977 6.97 -50.59 89.30 0.9999
12 8.52 -52.83 72.35 0.9802 2.31 -17.77 37.11 1.0000
13 4.02 -25.56 39.04 0.9896 2.93 -21.54 99.57 1.0000
14 6.34 -41.03 64.63 0.9950 1.63 -13.33 86.88 1.0000
15 5.93 -34.94 40.13 0.9905 2.55 -19.99 67.94 1.0000
16 6.11 -36.99 47.08 0.9722 2.85 -21.77 70.35 1.0000
Appendix I – Supplementary Data
115
Table 13. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (B3LYP/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 6.11 -40.88 68.95 0.9981 8.99 -63.78 124.20 0.9998
2 6.18 -41.38 69.78 0.9978 8.66 -61.83 121.34 0.9999
3 2.77 -14.73 10.60 0.9984 2.63 -19.68 73.61 1.0000
4 5.20 -34.42 57.00 0.9972 7.22 -51.48 125.71 0.9998
5 3.79 -20.13 14.64 0.9984 2.02 -15.67 67.25 1.0000
6 7.29 -46.46 70.62 0.9900 4.26 -32.20 95.89 1.0000
7 5.20 -34.42 57.04 0.9972 7.44 -53.15 137.63 0.9999
8 16.29 -108.65 180.38 0.9986 0.23 -2.08 140.37 0.9999
9 5.52 -35.22 54.19 0.9901 0.34 -2.88 122.95 1.0000
10 7.95 -53.04 88.76 0.9982 7.88 -57.50 147.77 0.9999
11 7.59 -50.54 83.87 0.9979 7.03 -51.35 109.29 0.9999
12 4.84 -28.47 32.59 0.9909 0.72 -6.79 40.43 0.9999
13 3.61 -23.10 35.70 0.9895 3.18 -23.33 119.54 1.0000
14 5.86 -38.12 60.76 0.9954 1.25 -10.87 99.52 0.9999
15 5.45 -31.99 35.80 0.9896 2.06 -16.62 77.16 1.0000
16 5.77 -35.04 44.74 0.9738 2.40 -18.73 80.11 1.0000
Appendix I – Supplementary Data
116
Table 14. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (LC-PBE/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 6.11 -40.86 68.72 0.9985 8.35 -59.03 103.83 0.9998
2 6.11 -40.86 68.71 0.9985 8.18 -58.14 102.65 0.9998
3 2.93 -15.78 12.06 0.9986 2.99 -21.97 64.67 1.0000
4 5.11 -34.02 56.50 0.9981 5.34 -38.06 88.83 0.9999
5 2.61 -12.63 2.85 0.9991 2.61 -19.65 61.18 1.0000
6 5.36 -33.87 50.46 0.9832 4.61 -34.36 85.92 1.0000
7 5.25 -34.78 57.54 0.9975 6.40 -45.61 111.28 0.9998
8 17.46 -116.06 191.31 0.9984 -0.04 -0.20 122.68 0.9997
9 6.32 -40.05 60.84 0.9881 0.17 -1.78 110.17 0.9998
10 7.70 -51.40 85.88 0.9982 7.42 -53.56 126.94 0.9999
11 7.43 -49.41 81.74 0.9979 7.06 -50.88 92.70 0.9999
12 5.18 -30.74 36.23 0.9893 1.92 -14.94 38.19 1.0000
13 3.75 -24.00 36.97 0.9922 2.96 -21.75 106.24 1.0000
14 5.84 -38.02 60.45 0.9962 1.54 -12.63 91.72 1.0000
15 5.52 -32.49 36.55 0.9903 2.86 -21.94 73.64 1.0000
16 5.77 -35.01 44.38 0.9709 3.09 -23.29 75.34 1.0000
Appendix I – Supplementary Data
117
Table 15. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (LC-PBE-D3/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 5.61 -36.78 60.15 0.9957 8.35 -59.03 103.83 0.9998
2 5.70 -37.19 60.41 0.9950 8.18 -58.14 102.65 0.9998
3 2.45 -11.88 3.89 0.9988 2.99 -21.97 64.67 1.0000
4 4.86 -31.39 49.96 0.9912 5.34 -38.06 88.83 0.9999
5 2.27 -9.48 -4.51 0.9994 2.61 -19.65 61.18 1.0000
6 5.20 -31.90 45.11 0.9422 4.61 -34.36 85.92 1.0000
7 4.79 -30.90 49.19 0.9921 6.40 -45.61 111.28 0.9998
8 18.61 -121.47 195.17 0.9970 -0.04 -0.20 122.68 0.9997
9 5.61 -33.99 47.51 0.9622 0.17 -1.78 110.17 0.9998
10 8.20 -53.65 87.14 0.9961 7.42 -53.56 126.94 0.9999
11 8.04 -52.37 84.22 0.9959 7.06 -50.88 92.70 0.9999
12 5.61 -32.69 37.37 0.9908 1.92 -14.94 38.19 1.0000
13 3.52 -21.69 31.35 0.9596 2.96 -21.75 106.24 1.0000
14 6.34 -40.46 62.49 0.9863 1.54 -12.63 91.72 1.0000
15 6.11 -35.36 38.95 0.9936 2.86 -21.94 73.64 1.0000
16 6.29 -37.49 46.29 0.9855 3.09 -23.29 75.34 1.0000
Appendix I – Supplementary Data
118
Table 16. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (CAM-B3LYP/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 5.61 -36.98 61.14 0.9963 -10.69 55.96 -63.08 0.9561
2 5.70 -37.54 62.01 0.9971 -11.62 61.38 -70.98 0.9553
3 2.27 -10.82 2.68 0.9989 -12.06 68.58 -63.97 0.9237
4 4.77 -31.00 50.02 0.9948 -11.68 63.51 -54.65 0.9465
5 3.95 -20.46 13.45 0.9986 -13.47 77.25 -77.11 0.9170
6 6.45 -40.19 58.71 0.9685 -24.41 139.96 -167.83 0.9151
7 4.93 -32.05 51.83 0.9956 -13.10 71.44 -56.33 0.9454
8 16.36 -107.80 175.74 0.9979 -5.32 31.28 83.70 0.8709
9 5.20 -31.95 46.05 0.9459 -6.02 35.24 61.38 0.8863
10 7.61 -50.21 82.69 0.9975 -15.52 84.24 -71.99 0.9510
11 7.36 -48.43 79.00 0.9967 -13.17 70.81 -81.88 0.9544
12 4.93 -28.51 31.26 0.9932 -11.08 63.10 -70.63 0.9291
13 3.27 -20.17 29.37 0.9569 -12.73 72.49 -28.91 0.9203
14 5.54 -35.39 54.82 0.9911 -13.21 75.66 -33.95 0.9243
15 5.27 -30.21 31.43 0.9950 -16.97 97.22 -97.67 0.9213
16 5.45 -32.33 38.81 0.9861 -14.34 81.48 -74.55 0.9285
Appendix I – Supplementary Data
119
Table 17. Polynomial fit information for the CP-corrected energy and the 13C isotropic
chemical shift vs the carbon tetrel bond length (BHandHLYP/6-311++G(d,p)).
𝑦 = 𝐀𝑥2 + 𝐁𝑥 + 𝐂
Energy
/ kcal/mol iso
/ ppm
Model A B C R2 A B C R2
1 5.77 -38.18 63.44 0.9973 8.46 -59.99 110.80 0.9998
2 5.95 -39.28 65.11 0.9972 8.24 -58.78 109.17 0.9999
3 2.43 -11.88 4.28 0.9990 2.93 -21.59 68.61 1.0000
4 4.91 -32.04 51.97 0.9952 6.70 -47.77 111.05 0.9999
5 3.12 -15.25 5.37 0.9988 2.48 -18.72 64.19 1.0000
6 6.04 -37.67 55.17 0.9719 4.70 -34.98 91.78 1.0000
7 4.84 -31.59 51.33 0.9946 6.96 -49.71 123.23 0.9999
8 16.61 -109.81 179.85 0.9981 0.20 -1.78 122.32 1.0000
9 5.20 -32.14 46.79 0.9630 0.36 -3.05 108.91 1.0000
10 7.70 -50.95 84.26 0.9972 7.77 -56.44 137.17 0.9999
11 7.86 -51.80 84.74 0.9980 7.73 -56.24 109.68 0.9999
12 5.02 -29.15 32.41 0.9934 2.01 -15.77 46.55 1.0000
13 3.34 -20.74 30.48 0.9662 3.19 -23.33 109.11 1.0000
14 5.68 -36.45 56.82 0.9919 1.92 -15.42 96.84 1.0000
15 5.34 -30.75 32.47 0.9943 2.86 -22.10 78.15 1.0000
16 5.61 -33.41 40.63 0.9877 3.11 -23.56 80.00 1.0000
Appendix I – Supplementary Data
120
Table 18. CP-corrected energy and the 13C isotropic chemical shift vs the carbon tetrel
bond angle (CAM-B3LYP/6-311++G(d,p)). In all cases the angle was set so that the
oxygen or nitrogen was placed between two methyl hydrogen atoms.
Interaction energy
/ kcal/mol iso
/ ppm
Model Structure Model Structure
Angle
/ degrees 12 13 16 12 13 16
140 -9.19 -0.73 -8.17 21.34 75.33 43.44
145 -9.34 -0.91 -8.33 20.88 75.14 43.07
150 -9.49 -1.08 -8.51 20.46 74.95 42.68
155 -9.64 -1.25 -8.69 20.09 74.78 42.31
160 -9.77 -1.40 -8.86 19.79 74.64 41.98
165 -9.88 -1.53 -9.01 19.56 74.54 41.72
170 -9.95 -1.63 -9.12 19.42 74.48 41.53
175 -10.00 -1.69 -9.19 19.36 74.48 41.42
180 -10.00 -1.71 -9.21 19.38 74.51 41.40
Appendix II – Sample of Computation Input Files
121
Appendix II – Sample of Computation Input Files
Gaussian Input for the Geometry Optimization of Acetylene
%nprocshared=4
%mem=200MW
%chk=acetylene.chk
# opt freq B3LYP/6-311++g(d,p)
Acetylene
0 1
O -2.38476950 0.11022044 0.00000000
C -3.64316950 0.11022044 0.00000000
C -4.15650238 0.79185828 1.28197473
H -3.79983653 1.80004974 1.31718059
H -5.22650238 0.79185682 1.28197551
H -3.79983440 0.25727357 2.13749044
C -4.15650310 -1.34082091 -0.05067148
H -5.22650116 -1.34089227 -0.04863256
H -3.80150292 -1.81380188 -0.94239110
H -3.79817192 -1.87595925 0.80380246
1 2 2.0
2 3 1.0 7 1.0
3 4 1.0 5 1.0 6 1.0
4
5
Appendix II – Sample of Computation Input Files
122
Gaussian Input for NMR calculation of Magnetic Shielding Contributions
%nprocshared=4
%mem=200MB
%chk=1.chk
# nmr lc-wpbe/6-311++g(d,p) empiricaldispersion=GD3
counterpoise=2 iop33(10=1)
Mag Sheild
0 1 0 1 0 1
C(Fragment=1) -0.02693000 -0.00289400 0.88347900
H(Fragment=1) -0.02717500 1.01401200 1.28351400
H(Fragment=1) 0.85369700 -0.51146400 1.28346400
H(Fragment=1) -0.90768000 -0.51156100 1.28308900
C(Fragment=1) -0.02685700 -0.00297000 -0.63762200
H(Fragment=1) 0.85055600 0.50421000 -1.04042300
H(Fragment=1) -0.02566900 -1.01586600 -1.04086500
H(Fragment=1) -0.90319800 0.50525200 -1.04080600
C(Fragment=2) -0.02729300 -0.00348000 -4.66034000
H(Fragment=2) -0.35968700 0.87559200 -5.24404400
H(Fragment=2) 0.30474000 -0.88301700 -5.24355300
O(Fragment=2) -0.02685700 -0.00297000 -3.46262200
Appendix II – Sample of Computation Input Files
123
Gaussian Input for NMR calculation of J-coupling
%nprocshared=4
%mem=200MB
%chk=2.chk
# nmr=spinspin cam-b3lyp/6-311++g(d,p) Counterpoise=2
J-coupling
1 1 1 1 0 1
C(Fragment=1) 3.54568454 0.01569282 0.23519796
H(Fragment=1) 3.91235854 0.89998582 -0.27818404
H(Fragment=1) 3.81597554 0.02344182 1.28480996
H(Fragment=1) 3.91092554 -0.87688118 -0.26470304
S(Fragment=1) 1.71996354 0.01562582 0.03088496
H(Fragment=1) 1.37618554 -0.97148218 0.88942096
H(Fragment=1) 1.37770954 1.01555082 0.87508296
N(Fragment=2) 6.46194146 0.01570318 0.46118604
C(Fragment=2) 7.60343946 0.01541618 0.51346204
H(Fragment=2) 8.67209546 0.01514518 0.56245804
1 2 1.0 3 1.0 4 1.0 5 1.0
2
3
4
5 6 1.0 7 1.0
6
7
8 9 3.0
9 10 1.0
10